This galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape, although not perfectly circular. There is a suggestion of a disk-like structure viewed at an oblique angle. The central bulge region is prominent and exhibits a reddish hue, possibly indicating an older stellar population. The outer regions of the galaxy display a greenish tint, potentially indicative of ongoing star formation or the presence of younger, hotter stars. Some minor irregularities are noticeable in the extended disk, hinting at possible past interactions or internal dynamical processes. The overall color profile suggests a mix of stellar populations and star formation activity across the galactic structure. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger, although some subtle disturbances cannot be ruled out.
