The galaxy appears as a relatively smooth, luminous spheroid with a slightly elongated morphology. It exhibits a dominant, concentrated central bulge and a fainter, diffuse halo. There is a possible faint, disk-like structure, but it is largely obscured or not well-defined in this image. The color suggests a stellar population that is moderately evolved, leaning towards older stars, possibly with an ongoing, but relatively subdued, star formation activity, as hinted by slightly bluer regions. There are some indications of minor disturbances, such as asymmetry or subtle tidal features, but the overall structure is consistent with an elliptical or S0 type galaxy. There is no clear evidence of a major ongoing merger. The overall roundness suggests a system nearing equilibrium.
