The galaxy presents a generally smooth, elliptical morphology. It appears relatively round, with a minor deviation towards a slightly elongated shape. The color profile suggests a mature stellar population, displaying a reddish-gold hue indicative of older stars. There is no visible spiral arm structure or significant dust lane obscuration. The galaxy appears undisturbed, with no obvious signs of recent or ongoing major mergers. Faint irregularities may suggest minor gravitational interactions, though these features are not prominent. Based on its apparent size and color profile, this galaxy is likely a massive elliptical galaxy with a relatively low star formation rate.
