The galaxy appears as a centrally concentrated object with a smooth morphology. The light distribution suggests a dominant spheroid component. It exhibits a slightly elliptical shape, tending more towards round than elongated. There is a distinct color gradient, with a yellowish-orange core that indicates an older stellar population dominating the central region. Fainter, bluer light is present in the outer regions, potentially indicating some ongoing, though relatively low, levels of star formation. There is no evidence of strong spiral arm structure or a distinct disk. No major mergers or significant tidal disturbances are visible.
