The galaxy appears to be a disk galaxy, exhibiting a flattened, elliptical shape. Its color profile suggests an older stellar population, with a dominant yellow-orange hue concentrated toward the center and a subtle bluish tint in the outer regions, possibly indicating some ongoing star formation, although the overall star formation rate seems low. The galaxy's smooth appearance indicates it has not recently undergone a major merger. There's no obvious presence of spiral arms, leading to a classification as a lenticular galaxy, which means it has a disk, but lacks prominent spiral structure. The central bulge is prominent and relatively bright, suggesting a high concentration of stars towards the core. The galaxy presents a moderate inclination to our line of sight, allowing a good view of its overall shape. Overall, the galaxy appears relatively undisturbed, settled in its environment with little signs of strong interactions with neighboring galaxies.