The galaxy presents a generally smooth and rounded morphology. Its light profile appears concentrated towards the center, suggesting a prominent bulge. The object exhibits a relatively symmetrical structure, with no apparent strong tidal features or major disturbances indicating ongoing or recent major merger activity. There are hints of a disk-like structure with faint arms or features.

The galaxy's color gradient shows a bluer color in the central regions, potentially indicative of younger stellar populations or ongoing star formation. The outer regions appear somewhat redder, which could imply older stellar populations or the presence of dust. Overall, the galaxy appears to be a relatively evolved system, potentially transitioning toward a more quiescent state of star formation. There is little evidence of active star formation, consistent with the observed smoothness and redder outer colors. The light seems quite concentrated within the central bulge.
