This galaxy exhibits an irregular morphology, showing signs of possible interaction or merger activity. A distinct, brighter central region is observed, suggesting a concentrated nucleus or bulge. The overall color of the galaxy appears to be yellowish-red, potentially indicating an older stellar population and/or significant dust content. There is a secondary, less prominent component or object located nearby, potentially a smaller galaxy in the process of merging, or tidal debris resulting from a prior interaction. The galaxy is not perfectly smooth; there appears to be some texture or patchiness, possibly due to ongoing or recent star formation. The outer regions are somewhat diffuse and lack a clearly defined boundary. Overall, the galaxy appears to be a massive system undergoing significant dynamical evolution.
