The galaxy presents a smooth, elliptical morphology, appearing relatively featureless. It exhibits a concentrated central bulge, indicative of an older stellar population. The color gradient suggests a dominant population of evolved stars. There is minimal evidence of spiral arm structures or significant dust lanes. No clear signs of recent or ongoing major mergers are apparent, though minor disturbances are not entirely excluded. The galaxy is relatively round in shape, lacking a highly elongated or cigar-shaped appearance. The overall light distribution is regular.
