The galaxy presents as a single, fairly symmetrical object. It appears to be an elliptical galaxy, characterized by a smooth, diffuse light distribution, lacking any prominent spiral arms or a distinct disk structure. The central region is brighter and exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions fade into a bluer color, possibly indicating some more recent, though subdued, star formation activity. No obvious tidal tails, strong asymmetries, or signs of a major ongoing merger are visible. There might be a slight warp on one side, possibly a minor disturbance. Overall, the galaxy appears relatively undisturbed and relaxed in morphology.
