The galaxy presents as a single, concentrated body of light. There is a distinct central bulge that appears relatively smooth and elliptical in shape. The galaxy exhibits a concentrated luminosity profile, with the brightest region located in the center, suggesting a high density of stars and potentially a supermassive black hole. 

No spiral arm structure or dust lanes are clearly visible in this image. The galaxy's color is predominantly yellowish-white at the core, transitioning to a slightly bluer hue in the outer regions. This color gradient may indicate a difference in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars populating the outskirts. The overall smooth appearance indicates a relatively relaxed and evolved system with a notable absence of active star formation regions. The estimated size is about 6.6 kiloparsecs in radius.
