The galaxy presents as a lenticular or early spiral type system, characterized by a prominent bulge and a disk. The bulge appears relatively smooth and spheroidal, exhibiting a concentrated luminosity profile towards the center. The disk component shows a faint, somewhat diffuse structure, lacking distinct, well-defined spiral arms.

The overall color of the galaxy indicates a mix of stellar populations. The central bulge displays a slightly yellower hue, suggesting a population of older, redder stars. The disk exhibits a bluer tint, hinting at the presence of younger, hotter stars and ongoing star formation.

There is some evidence of a possible minor disturbance or asymmetry in the disk region. A slight irregularity in the light distribution on one side of the galaxy may suggest gravitational interaction or recent minor merger activity. However, this feature is subtle and requires further investigation.

The galaxy's morphology suggests that it is in a transitional phase, evolving from a spiral-rich morphology toward a more lenticular, gas-poor state. It is estimated to be roughly 4 kpc in radius, exhibiting a modest luminosity, and moderate stellar mass. Based on its color and morphology, it likely exhibits a low rate of star formation.
