The galaxy presents as a concentrated, predominantly smooth object. The color profile exhibits a central yellowish-orange hue, indicative of an older stellar population dominating the core. There appears to be a subtle color gradient from the center towards the outer regions, shifting towards a slightly bluer, less intense coloration, which may suggest the presence of younger stars and/or ongoing star formation in the outer regions, albeit at a low rate. The overall morphology appears largely undisturbed, displaying no immediately apparent signs of major mergers or tidal disruptions. The galaxy’s shape approximates a round form. There are suggestions of a minor asymmetry or subtle feature in the outskirts of the galaxy but resolution is limited.
