The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The overall shape is quite round, showing minimal elongation or distortion. There is no visual evidence of spiral arm structure or significant dust lanes. Its color profile appears to be somewhat redder than typical spiral galaxies, suggesting a population of older stars and a relatively low rate of ongoing star formation. There are no obvious signs of a major ongoing merger or tidal disturbances in this image, although minor asymmetries or subtle disturbances may be present at levels below the image resolution.
