The object presents as a roughly elliptical galaxy with a concentrated central bulge. The core region exhibits the highest luminosity, appearing almost uniformly bright. The surrounding galactic disk shows a noticeable color gradient, transitioning from a brighter, potentially younger stellar population in the inner disk to a more diffuse, fainter outer region. Some subtle structural features, potentially indicative of minor tidal disturbances, are present within the disk, though the overall morphology appears largely undisturbed. There is an indication of an inner ring around the bright core, though it is fragmented. Based on its overall morphology and colors, this galaxy is likely a relatively massive system, possibly an elliptical galaxy in the early stages of a minor merger or tidal interaction. Further analysis is required to accurately ascertain its precise type, evolutionary state, and the nature of any observed disturbances.
