The galaxy presents a generally smooth morphology, with a high probability of being classified as such. It appears elliptical in shape, with an aspect ratio that is close to round, but trending towards an in-between classification as opposed to perfectly circular or highly elongated. There is some indication of internal structure, although it is not strongly pronounced and could be subtle dust lanes or minor irregularities. There are no obvious signs of tidal tails or other indications of a major ongoing merger. The galaxy has a redder color profile, suggesting an older stellar population and a low rate of star formation. The overall color index suggests relatively little ongoing star formation.
