The galaxy presents as a singular, relatively smooth and rounded object. The overall color profile leans toward a warmer palette, with a concentrated yellowish-orange core that gradually diffuses outwards. This core suggests a higher concentration of older stars and possibly a supermassive black hole at the galactic center. The galaxy exhibits a noticeable lack of spiral arm structure or dust lanes, implying that it may be an elliptical galaxy or a lenticular galaxy viewed nearly face-on. The outer regions of the galaxy display a slightly cooler tone, tending towards a pale green or yellow hue, indicating a population of younger stars in the outer regions, though the overall star formation rate appears to be relatively low. There's no visual evidence of ongoing major mergers or significant tidal disturbances, suggesting that the galaxy is in a relatively quiescent state. The galaxy appears relatively isolated, without any immediately obvious signs of interaction with neighboring galaxies.
