This galaxy presents as a generally smooth, elliptical-like object with a noticeable central bulge. The core region exhibits a bright, concentrated luminosity, suggesting a higher density of stars within the nucleus. There is a gradual decrease in luminosity observed as one moves away from the center, with a seemingly even distribution of light throughout. The overall shape is somewhat elongated but not highly flattened, tending towards a more spheroidal morphology. The color profile appears to be dominated by yellowish hues, which is indicative of an older stellar population. There is little to no evidence of spiral arms, dust lanes, or other distinct features typically associated with younger, star-forming galaxies. Possible minor distortions are not clearly detected, and there is no obvious indication of any ongoing mergers or major tidal disturbances, which could contribute to the galaxy's morphology.
