The galaxy presents a somewhat elliptical morphology, though it appears more disc-like. It displays a concentrated central bulge exhibiting a yellowish hue, possibly indicating an older stellar population. The outer regions exhibit a bluer tint, suggestive of younger stars and ongoing star formation, though it does not appear very active. There's a subtle irregularity in the disk, suggesting a possible minor disturbance or interaction. The galaxy appears to be moderately massive, and its star formation rate is relatively low. The overall appearance suggests a galaxy that is transitioning from a more active, star-forming state to a more quiescent one.
