The galaxy presents as a relatively smooth, elliptical structure with a prominent, bright central bulge that appears nearly spherical. The overall shape is somewhat elongated, tending toward a cigar-like appearance. There is a subtle, disk-like structure surrounding the bulge. The galaxy exhibits a color gradient, with the central bulge appearing more yellowish-white, indicating an older stellar population. The outer regions are slightly bluer, suggesting the presence of younger stars and ongoing, or recent, star formation. There are no obvious signs of major disturbances due to merging events; the galaxy appears relatively undisturbed. Subtle irregularities are seen in the disk, potentially minor tidal features. Overall, the galaxy appears to be an intermediate mass system with an active star formation rate.
