The galaxy presents a smooth, elliptical morphology, characterized by a centrally concentrated light distribution. It displays a color gradient, with the core exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions appear slightly redder, potentially indicating a higher proportion of dust or cooler stars. A minor asymmetric feature is detected, potentially indicative of a small interaction. The galaxy exhibits a relatively high degree of radial symmetry, and does not obviously present spiral arms.
