The galaxy presents as an elliptical or lenticular-like structure with a smooth, diffuse morphology. The central region exhibits a significantly higher surface brightness, appearing as a concentrated and luminous core. Progressing outwards from the core, the luminosity gradually decreases, resulting in a somewhat indistinct outer boundary. There is subtle hint of disturbance in the system. The overall color is suggestive of an older stellar population, and the estimated size suggests that it is a fairly substantial galaxy.
