The galaxy presents a largely smooth morphology, with a slight hint of disk-like structure. It appears to be somewhat elongated, but is mostly rounded. The light distribution appears concentrated towards the center, but the distribution is fairly smooth overall. The galaxy has a distinct color gradient, transitioning from a bluer hue at its outer edges to a yellower, more reddish color towards its core, potentially indicating a differential distribution of stellar populations, with younger, bluer stars in the outer regions and older, redder stars concentrated in the bulge. There is a hint of some disturbance present, although not major. The galaxy exhibits a moderate degree of asymmetry in its light distribution.
