The galaxy appears as a fairly elliptical, though slightly irregular, spheroid of light. Its core is a bright, diffuse yellow-orange, which gradually fades into a less intense halo. There are only faint signs of structure in the halo, likely it is mostly smooth. There appears to be no significant disk component. Based on its morphology, it may be a relatively massive, quiescent galaxy with very little active star formation, likely dominated by an older stellar population. However, a slight asymmetry is visible in the halo's outer edges, which could be indicative of a past or ongoing minor merger event, or some internal disturbances in the galaxy.
