This galaxy presents as a resolved, though somewhat diffuse, object. It exhibits a morphology that appears to be predominantly smooth, suggesting it may be an elliptical galaxy, though there is some indication of a very weak disk-like structure or possible tidal disturbances.

The color profile shows a central yellowish concentration, potentially indicating an older stellar population dominating the core, with relatively little ongoing star formation. The outer regions display a bluer hue, hinting at the presence of younger, hotter stars or perhaps recent or ongoing star formation in those areas. The object exhibits a relatively regular, almost circular shape. There appears to be no significant signs of major mergers or tidal interactions at this resolution, though there might be subtle disturbances indicating minor past or current interactions.
