The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The core presents a yellowish-orange hue, suggesting a population of older stars. The outer regions of the galaxy exhibit a gradual decline in luminosity, transitioning into a faint halo. There is a slight asymmetry in the color distribution, hinting at possible tidal interactions or subtle disturbances. Overall, the galaxy appears to be relatively isolated and mature.
