The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution appears fairly uniform, with a gradient towards the center, suggestive of an older stellar population. There is a subtle color variation, with the central region appearing more yellowish, potentially indicating a higher concentration of evolved stars. No spiral arms or distinct features are immediately apparent, consistent with a classification leaning towards an early-type galaxy. The overall morphology suggests a system that has largely completed its major star formation phase. There is no obvious evidence of any major ongoing mergers or strong tidal disturbances.
