The galaxy presents as a centrally concentrated, relatively smooth object. Its overall shape appears mostly round, with no obvious spiral arm structures or bar features visible. The color profile suggests a population of older stars, with a predominantly yellowish hue dominating. There is a slightly bluer coloration in the central region, which may indicate some ongoing, albeit low-level, star formation activity. No significant tidal features, dust lanes, or signs of a recent major merger are immediately apparent. Subtle asymmetries could indicate minor gravitational interactions, but further investigation is required. The galaxy's smooth morphology suggests it could be an elliptical galaxy or a lenticular galaxy seen face-on.
