The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, deviating slightly from a perfect circle. The light profile suggests a bulge-dominated system, with a gradual decrease in luminosity outward from the core. The color is generally yellow, hinting at an older stellar population with a moderate level of star formation. There is no evidence of significant spiral arm structure, tidal features, or ongoing major mergers. Subtle disturbances cannot be ruled out.
