The galaxy presents as an elliptical morphology, appearing moderately smooth with a dominant central bulge. The bulge exhibits a concentrated luminosity, transitioning to a less luminous, more diffuse halo. There is a slight elongation of the galaxy's shape, suggestive of a mild cigar-shaped structure, though it primarily presents as in between round and elongated. No distinct spiral arm structures or significant dust lanes are discernible in the image. The overall color appears to be on the redder side, indicating an older stellar population and potentially lower star formation activity within the galaxy. Faint asymmetrical distortions hint at possible minor gravitational interactions or past merger events.
