This galaxy appears to be a relatively compact system. It displays a dominant, roughly spherical central bulge with a smooth, diffuse light distribution. The color of the bulge is predominantly yellowish-orange, suggesting an older stellar population. Fainter features are present around the brighter central area. There are also several regions of active star formation, indicated by the localized bluer regions of light. These areas are primarily distributed in what may be distorted arm segments or tidal features, implying potential gravitational interactions with another galaxy. The galaxy as a whole lacks a clear disk structure and might be classified as an elliptical galaxy or potentially a spiral galaxy undergoing a merger or significant tidal disruption.
