The galaxy presents an elliptical morphology, appearing somewhat elongated with a noticeable central bulge that dominates the luminosity profile. The bulge exhibits a smooth, concentrated light distribution. The outer regions of the galaxy appear fainter with a less defined structure, suggesting a gradual decrease in stellar density. The overall color of the galaxy is on the redder side, indicative of an older stellar population. The disk appears diffuse, lacking prominent spiral arm structures. There is a slight asymmetry in the galactic disk with hints of a subtle warp.
