The galaxy appears as an elliptical or lenticular-type system, exhibiting a smooth, centrally concentrated light profile. There is a clear, bright core region. The galaxy appears flattened, suggesting some degree of rotation. The system shows a slightly elongated morphology, appearing more "in-between" round and cigar-shaped. There does not appear to be a strong presence of spiral arms or significant dust lanes. The overall color suggests that the galaxy contains an older stellar population. There are no obvious signs of strong tidal interactions or major mergers. However, the galaxy's moderately disturbed structure is suggestive of some past interactions. Star formation is likely ongoing, but at a low rate.
