The galaxy presents as a generally smooth and concentrated distribution of light. It exhibits an elliptical morphology. There is a bright, concentrated central bulge, fading into a more diffuse halo. The galaxy appears to be relatively undisturbed, without any obvious signs of tidal features or major asymmetries indicating a recent merger event. There is a slight elongation, giving it a slightly cigar-shaped appearance. The color appears to be redder and more concentrated towards the center, suggesting an older stellar population in the core, with bluer, younger stars possibly contributing to the fainter outer regions.
