The galaxy presents as a relatively smooth, elliptical structure. Its core appears as a concentrated, bright yellowish-orange region, suggesting an older stellar population. Surrounding this core is a more diffuse halo of greenish light, possibly indicating the presence of ionized gas or a younger stellar population experiencing some star formation, although at a low rate. The overall shape of the galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal disruptions. The galaxy exhibits a moderate degree of roundness, closer to a circular shape than an elongated, cigar-like form. No significant dust lanes or prominent spiral arm structures are discernible within the galaxy's observed morphology. Overall, it seems to be an early-type galaxy with characteristics consistent with an aging population.