The galaxy presents as a well-defined elliptical type with a smooth, featureless morphology. It exhibits a high degree of central concentration, as evidenced by a bright, nearly circular core that fades gradually into the surrounding halo. The galaxy appears fairly round. The lack of discernible spiral arms or dust lanes suggests that this is an older system, potentially with minimal ongoing star formation. The color profile is generally reddish, which is consistent with a stellar population dominated by older, redder stars. There is no apparent evidence of any significant merging activity or major disturbances impacting its overall structure.
