The galaxy appears to be a luminous elliptical or S0 type galaxy, exhibiting a smooth, centrally concentrated morphology. The light distribution suggests a relatively old stellar population, with a yellowish-white hue dominating the central bulge. There's little to no evidence of spiral arms or significant dust lanes. The galaxy presents with high degree of roundness. There might be slight asymmetry or a minor tidal feature suggesting a previous interaction. Overall, the galaxy presents as a relatively undisturbed system in terms of any major ongoing mergers. The estimated size indicates it's of moderate size. Based on the galaxy's color and morphology, it is likely to have a low star formation rate.
