The galaxy appears as a largely smooth, centrally concentrated object with a near-circular morphology. There is little evidence of spiral arm structure or significant disk-like features. The galaxy exhibits a bright central region, with a gradual decrease in luminosity towards its outer edges. The color profile suggests a dominant population of older stars, with a somewhat bluer hue in the very center. The overall appearance is consistent with an elliptical galaxy, possibly an early-type spiral viewed at a high inclination. There may be a faint indication of a slight asymmetry or minor disturbance in the outer regions, but the overall structure remains largely undisturbed.
