The galaxy presents as a relatively compact, luminous structure. It exhibits an elliptical morphology, appearing significantly more elongated in one dimension than the other. The color profile is predominantly yellow-orange, suggesting an older stellar population and potentially a lower rate of ongoing star formation. There is a hint of disk-like structure, possibly indicative of a transition from a more active spiral galaxy to a lenticular or elliptical morphology. There is also evidence of a potential interaction or merger event occurring, based on the apparent irregular structure and the possible presence of tidal features. These features include faint, diffuse extensions that could be the remnants of a recent galactic merger or ongoing tidal interactions with a neighboring galaxy. The galaxy appears to be a relatively massive system, based on its luminosity and estimated size. Overall, the galaxy appears to be a massive, relatively evolved system undergoing morphological transformation, potentially as a result of galactic interactions.
