The galaxy presents as an elliptical type, exhibiting a centrally concentrated luminosity profile. The core is bright and yellowish-white, suggesting a population of older stars. Moving outward from the core, the galaxy displays a diffuse, spheroidal halo with a subtly fainter, reddish-orange hue, indicative of an aging stellar population. There is a general smoothness to the galaxy's structure with no obvious spiral arm structures or strong dust lanes visible in the image. The light distribution appears to be fairly uniform across the galaxy, with a gradual decrease in brightness from the center to the outer edges. There is no evidence of major tidal disturbances or active galactic nuclei features discernable within this image.
