The galaxy presents as a relatively smooth, elliptical structure. A concentrated, bright central bulge dominates the galaxy's morphology, exhibiting a yellowish-white hue. The bulge transitions into a fainter, more diffuse halo extending outwards. There is subtle evidence of a flattened disk-like structure surrounding the central bulge, indicated by a slight elongation. Some bluer regions are observed in the outer parts, suggesting recent star formation. The galaxy appears relatively isolated with no obvious signs of interaction with neighboring galaxies, although some minor disturbances cannot be ruled out. Overall, the galaxy is estimated to have a large mass and a moderate rate of star formation.
