This galaxy appears to be an elliptical or lenticular galaxy, as its morphology is largely smooth with a relatively high degree of central concentration. The light profile is dominated by an ellipsoidal component, with the isophotes transitioning from a rounder shape in the inner regions to a more elongated, cigar-like shape in the outer regions. The color gradient indicates that the central region is redder than the outer disk. A slight blue tinge around the outer edges may indicate some low-level star formation in those areas. There is no evidence of strong spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of major interaction or merging events, although there could be a minor disturbance due to a smaller object.
