The galaxy presents as a relatively smooth, elongated structure. It is likely an elliptical galaxy due to its lack of apparent spiral arms or a distinct disk-like morphology. The central region exhibits a brighter, more concentrated luminosity, suggesting a higher stellar density. The outer regions of the galaxy gradually fade into the background sky. There appears to be very minimal evidence of active star formation, inferred from the relatively smooth color gradient and lack of patchy, blue regions. The morphology suggests the galaxy has undergone significant evolutionary processing, such as mergers, leaving it with a spheroid shape. There is no immediate visual indication of a major ongoing merger or significant tidal disturbances; however, a very slight irregularity can be observed suggesting that perhaps minor interactions or minor mergers may have played a role.
