The galaxy appears as a moderately bright, elliptical object with a smooth, relatively featureless morphology. Its color index indicates a redder overall composition, suggesting an older stellar population with limited ongoing star formation. The shape appears fairly round, with a high degree of central concentration and a gradual decrease in luminosity towards its outer edges. There is some indication of potential tidal interactions or minor disturbances in the galaxy's structure, particularly with a merging fraction observed, possibly suggestive of past or ongoing interactions with other galaxies, however, the details are not clear from this image. Its estimated size suggests that it is a relatively large galaxy. The galaxy's absolute magnitude confirms a high intrinsic luminosity.
