The galaxy presents as a generally smooth, elliptical-like object. There is a concentration of light towards the center of the galaxy, suggesting a bulge. The color gradient appears redder towards the center, indicating a population of older stars, and bluer towards the outer regions, potentially indicating regions of more recent, though subdued, star formation. There is no strong indication of spiral arm structure or a distinct disk. The galaxy appears relatively isolated, showing no obvious signs of major mergers or tidal disturbances, though a minor interaction cannot be ruled out based solely on the image. The overall morphology suggests a system evolving towards quiescence.
