The galaxy presents as a centrally concentrated spheroid with a noticeable radial gradient in luminosity. The core region exhibits a high surface brightness, appearing a yellow/gold hue. Moving outward from the core, the light gradually diffuses into a less luminous halo.

Based on its morphology, the galaxy is likely an elliptical type, exhibiting a smooth profile. There are no visible spiral arms or a prominent disk structure. Given its color profile, the stellar population is presumed to be dominated by older stars, potentially with ongoing star formation. No clear signs of recent or ongoing major mergers are observed. The galaxy appears relatively isolated.