The galaxy presents as an elliptical morphology, with a relatively smooth light distribution across its body. The core is bright and concentrated. There is a prominent central bulge that dominates the overall structure. 

There appears to be a slight asymmetry in the outer regions and some very faint diffuse features. The asymmetry is most visible on the right side of the galaxy, where there is a bright, slightly irregular feature that appears distinct from the main body, suggesting a potential interaction or tidal disturbance.

The galaxy's color suggests the presence of an older stellar population, with a tendency towards redder hues in the central regions, potentially indicating the presence of evolved stars. There appears to be active star formation in the disturbed regions.
