The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The shape is more of an oblate spheroid than a perfect sphere. Faint, diffuse extensions are present surrounding the main body of the galaxy, which may be indicative of a tenuous halo. There may be a slight blue tinge in the arms of the galaxy, which could indicate recent star formation. There does not appear to be any ongoing major merging activity or obvious tidal disturbances. Overall, the galaxy is consistent with an early-type morphology.