The galaxy presents as a somewhat elliptical, disk-like structure with a smooth overall appearance. Its core exhibits a bright, concentrated luminosity, suggesting a significant density of stars or potentially an active galactic nucleus. The galaxy displays a subtle color gradient, shifting from a yellowish-white hue at its center to a slightly bluer tint in the outer regions of the disk. This color variation may be indicative of differing stellar populations, with older, redder stars concentrated centrally and younger, bluer stars populating the periphery.

There are signs of minor irregularities or disturbances in the disk's morphology, possibly resulting from a past or ongoing interaction with another galaxy. A faint, diffuse halo extends beyond the main body of the galaxy, contributing to its overall extent. This halo appears relatively smooth and featureless. The lack of prominent spiral arms or other distinct features suggests that this is an evolved system.
