This galaxy appears to be an elliptical galaxy, displaying a largely smooth and rounded morphology. There is little to no evidence of spiral arms or a distinct disk structure. The color profile suggests an older stellar population, with a yellowish hue dominating the central region. The galaxy appears relatively isolated, showing no obvious signs of major mergers or significant tidal disturbances, although the image resolution is limited. No visible dust lanes or prominent star-forming regions are discernible. Based on its apparent smooth shape and color, the galaxy is likely comprised primarily of older stars. The light is concentrated in the central region, with a gradual fading toward the outer edges.
