The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Extending outwards from the central region, the galaxy displays a more diffuse, bluish halo, which could indicate the presence of younger stars or ongoing star formation, although limited. The overall shape deviates slightly from a perfect circle, appearing somewhat elongated, tending toward a cigar shape. There appears to be no signs of major mergers or significant tidal disturbances, however, a slight asymmetry in the outer regions hints to a possible minor interaction. 
