The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated brightness, suggesting a high stellar density or possible active galactic nucleus. There is a noticeable flattening, with the shape being somewhere between round and elongated. Hints of fainter, diffuse material extend outwards from the central region, giving the galaxy a fuzzy appearance and indicating the presence of an extended halo. There is a possible minor disturbance in the halo or at the very edge of the galactic disk, though a merging event is unlikely. Overall, the galaxy appears to be relatively quiescent, based on the lack of strong spiral arms or prominent star-forming regions.
