The galaxy presents a flattened, elliptical morphology. The light distribution appears smooth and centrally concentrated, suggesting a dominant bulge component. The overall color is yellowish-orange, with a subtle reddish tint in the central region. This color profile implies a stellar population dominated by older stars.

There is no apparent spiral arm structure, although the smooth appearance of the galaxy could be obscuring such features. The lack of distinct dust lanes or patches is also consistent with a population of older stars. The galaxy has a moderate size and is of a significant mass. There is no evidence of a recent or ongoing major merger. A minor disturbance cannot be ruled out.