The galaxy presents as a relatively smooth, elliptical-like object. A bright central bulge dominates the light profile, suggesting a high concentration of older stellar populations. The outer regions of the galaxy exhibit a fainter, more diffuse halo. There is a subtle color gradient, with the core appearing slightly bluer than the outer regions, which have a more reddish hue. This might indicate some level of ongoing star formation, though it appears to be more active in the central regions. There is no evidence of spiral arms or a well-defined disk structure. There are no clear signs of any major mergers or tidal disturbances affecting the galaxy's overall morphology, although some subtle irregularities in the outer regions might be present. Overall, the galaxy appears to be a quiescent, relatively isolated system.
