The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright yellow glow. The isophotes appear generally circular, suggesting minimal rotational support. There is a slight elongation that can be observed. The overall color index suggests a population dominated by older stars. There are no prominent dust lanes, spiral arms, or other features indicative of recent major merger activity or significant ongoing star formation. The galaxy does not appear to be experiencing any active mergers. The lack of distinct features indicates a relatively quiescent state.