The galaxy appears as a moderately bright, slightly elongated object. It exhibits a dominant central bulge. The primary color is a bluish-white, suggesting the presence of a relatively young stellar population. A very faint disk is present, displaying minor structural disturbances, possibly indicating a minor merger. The overall morphology suggests a galaxy in transition, neither purely elliptical nor a fully developed spiral. There may be some on-going, albeit limited, star formation activity, as indicated by the subtle blue hues, concentrated centrally.