This galaxy presents as a somewhat elliptical structure with a smooth, diffuse appearance. The central region exhibits a concentration of light, appearing yellowish-orange, indicative of an older stellar population and potentially a bulge component. The outer regions of the galaxy appear less luminous and have a slightly bluer hue, suggesting the presence of younger, hotter stars and possible ongoing, but likely subdued, star formation. There appears to be a slight hint of a disk-like structure, though no spiral arms are clearly visible. The overall shape leans more towards elliptical than a flattened disk, and there are no obvious signs of major tidal disturbances or ongoing mergers, although some subtle irregularities in the outer regions might suggest a past minor interaction. The galaxy's smooth texture suggests a relatively well-mixed stellar population.
