This galaxy exhibits a centrally concentrated structure with a smooth, elliptical morphology. The core region displays a bright, whitish-blue hue, suggestive of a population of relatively young, hot stars or potentially an active galactic nucleus, though the resolution is insufficient to confirm the latter. The isophotes are generally regular, although there appears to be a slight elongation. There is a faint reddish component visible peripherally. A small disturbance may be present, but the data is not of sufficient quality to confirm interaction or merging activity. Overall, the galaxy appears to be a relatively massive system with moderate star formation activity.
