The galaxy presents as a relatively compact structure with a somewhat indistinct morphology. A dominant, smooth component is observable, with a centrally concentrated luminosity profile. There is a marginal indication of a disk component that is hinted at within the image, the galaxy does not appear to have any spiral arm structure and presents as smooth. It is likely that the system is undergoing a minor disturbance due to merger activity, based on observed asymmetries. The central bulge region appears relatively indistinct. The overall color profile is consistent with an older stellar population, potentially with an ongoing low level of star formation. The galaxy does not present an obviously rounded shape, and the shape observed appears to be in between rounded and elliptical.
