The galaxy presents a generally smooth morphology, with a concentrated central bulge. The shape is largely elliptical, appearing neither perfectly circular nor significantly elongated. Faint, diffuse features surround the central bulge, suggesting a possible disk-like structure, or a more diffuse halo of stars. The color profile indicates a redder core, shifting to slightly bluer hues in the outer regions. This suggests that the central region is dominated by older stellar populations while the outer regions have undergone more recent episodes of star formation. There are no obvious signs of major mergers or tidal disturbances. However, slight asymmetry in the outer regions hints at minor gravitational interactions.
