The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, appearing brightest towards the core region. There is a noticeable color gradient, shifting from a yellowish-white hue in the central bulge to a slightly redder tint in the outer regions. The ellipticity is moderate, not appearing perfectly spherical but not highly elongated either, somewhere in between round and cigar shaped.. No distinct spiral arms or prominent dust lanes are discernible in this image. The overall appearance suggests a mature stellar population with a possible lack of ongoing major star formation. There may be minor disturbances in the structure, but no signs of a major ongoing merger.
