The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a high degree of central concentration with a bright core that gradually fades into the surrounding halo. The main body of the galaxy presents an overall rounded morphology. There is no obvious presence of spiral arms or a prominent disk. The color distribution suggests a stellar population dominated by older, redder stars, particularly within the central region, although some bluer components are visible in the outskirts. There are no apparent signs of major ongoing mergers or significant tidal disturbances. The galaxy exhibits a minor disturbance with a likely merger event that appears to be nearing completion.
