The galaxy appears as a centrally concentrated object with a generally smooth morphology. A slightly elongated shape is visible, though the galaxy tends more towards round. The central bulge appears bright and moderately compact, with a gradual decrease in luminosity towards the outer regions. There is a hint of a disk component. Overall, the galaxy presents a relatively undisturbed structure, with no strong evidence of major mergers or significant tidal interactions. The color profile suggests a population of older stars dominating the light output. The galaxy exhibits a diffuse halo with very faint outer regions.