The galaxy appears as a relatively smooth object, with a mostly elliptical morphology. It exhibits a moderate degree of ellipticity, appearing more in between round and cigar shaped. There are no strong indications of spiral arms or a well-defined disk structure; however, there seems to be some evidence of a weak disk. The galaxy's light profile suggests a centrally concentrated luminosity distribution. The object's color indicates the presence of an older stellar population. There may be an indication of some minor gravitational disturbance, but it could be a merger candidate based on light distribution. There does not appear to be any prominent tidal tails or other signs of ongoing major merger activity. Star formation activity is low.
