The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There is a lack of discernible spiral arm structure or prominent dust lanes, although faint, irregular extensions of the main body may be present. The galaxy's light profile indicates a gradual decline in intensity from the core outward, suggesting a diffuse halo component.

Color gradients are subtle, with a slightly bluer hue in the outer regions of the galaxy and a reddish tone towards the center, consistent with a population of older stars. The overall color suggests a galaxy dominated by evolved stellar populations, yet the star formation rate is non-negligible. The galaxy exhibits minimal signs of tidal disturbances or interactions with other galaxies.
