The galaxy presents as a lenticular-shaped object with a smooth, centrally concentrated luminosity profile. The primary axis of the galaxy is clearly defined, with an ellipticity suggesting a significant inclination relative to our line of sight. There is no obvious spiral arm structure or prominent dust lane visible. The galaxy core is moderately bright, and the overall color appears to be subtly redder in the central regions, potentially indicative of an older stellar population. The outer regions of the galaxy exhibit a more diffuse, fainter glow, with no sharp cutoff in luminosity. Faint traces can be observed on the furthest extents of the galaxy suggesting the presence of a disk.
