This galaxy presents a generally smooth morphology. The overall color gradient shifts from a bluer periphery toward a more yellow-white core, suggesting an aging stellar population concentrated in the galactic center. A slight elongation is observed in the shape, transitioning from round to a more cigar-shaped form. Some minor disturbances are apparent, indicating possible past interactions or internal dynamical processes. There is no clear evidence of a strong spiral structure or bar. The galaxy appears relatively isolated, without obvious signs of ongoing major merging activity. Star formation appears subdued, as indicated by the less prominent blue color in the galaxy.