The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears largely elliptical, with a high degree of roundness. The central region exhibits a bright, yellowish core. The color profile is dominated by redder wavelengths, with hints of green within the diffuse outer regions. No spiral arm structure or significant dust lanes are discernible. There is no visual evidence of strong tidal features or ongoing major merger activity, although subtle irregularities in the outer isophotes may suggest minor gravitational disturbances. Based on these characteristics, the galaxy likely represents a relatively massive system with a moderate star formation rate.