The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish-orange hue, suggestive of an older stellar population, but also has several bluer areas, indicating younger stars or areas of active star formation. There are slight signs of disturbance in its morphology, possibly indicative of past minor interaction or internal dynamic processes. The galaxy appears relatively isolated with no immediately apparent major merger events influencing its shape, but the existence of tidal tails cannot be ruled out. There are some visible irregularities in the galactic disk, possibly spiral structures, though the smoothness suggests the spiral arms are tightly wound. Overall, the galaxy appears to be transitioning from an active star-forming phase to a more quiescent state dominated by older stars.
