The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. Surrounding the core, there is a fainter, more diffuse halo of similar color, suggesting a gradual decrease in stellar density with radial distance. There is very faint evidence of a very small disk. The overall color suggests this is a galaxy with little active star formation. There's no visually apparent spiral structure or significant dust lanes. Overall, the galaxy appears to be isolated and undisturbed, with no obvious signs of ongoing or recent mergers.