The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated light profile, with luminosity decreasing gradually outward from the core. The overall color is somewhat reddish, suggestive of an older stellar population and diminished current star formation. The morphology is largely undisturbed, with no obvious signs of ongoing mergers or significant tidal interactions. The galaxy's shape appears close to circular, lacking a pronounced disk-like structure or strong asymmetry. There is very little, if any, evidence of spiral arms or distinct star-forming regions. The galaxy's color suggests it may reside on the red sequence.
