The galaxy exhibits a generally smooth morphology. Its overall shape appears to be elliptical or spheroidal, displaying a high degree of roundness. There is no clear evidence of spiral arms or a prominent disk structure.

The galaxy displays a distinct color gradient, with a bluer core and redder outer regions. The bright central region exhibits a cyan hue, suggesting the presence of hotter, younger stellar populations or possibly an active galactic nucleus. Moving outwards, the color transitions to a more yellow/orange appearance, indicating a population of older, cooler stars.

There is a hint of a possible minor disturbance or interaction based on a slight asymmetry in the outer regions of the galaxy, as well as a slight haze surrounding it.
