The galaxy presents as an elliptical structure with a significant central bulge. The core exhibits a bright, yellowish-white hue, suggesting a high concentration of older stars. There is a lack of discernible spiral arm structure or dust lanes. The light distribution is relatively smooth and symmetrical. The galaxy appears elongated, possibly cigar-shaped, indicating an oblate spheroidal morphology viewed at an angle. There is no evidence of major merger events or tidal tails. Faint extensions are visible at the edges of the galaxy, suggesting a diffuse halo component. Overall, the galaxy seems to be an evolved system with suppressed star formation activity.
