The galaxy presents as a relatively compact, yet luminous object. Morphologically, it appears to be a system undergoing some level of interaction or disturbance. The central region exhibits a slightly irregular shape, potentially indicating an ongoing merger event or tidal interactions. The light distribution is mostly smooth, suggesting a evolved stellar population, but there are hints of patchy areas or minor extensions emanating from the core. The color profile appears to be redder throughout with some localized regions which may indicate recent or ongoing star formation. Overall, the galaxy appears to be a massive, relatively evolved system experiencing mild interactions, possibly leading to a merger.
