The galaxy presents as a centrally concentrated elliptical form, with a smooth, largely featureless appearance. The core region exhibits a strong, bright, yellowish hue suggesting an older stellar population. Moving outwards from the core, the light gradually fades, transitioning to a fainter, more diffuse envelope that has a slightly bluer tint relative to the central bulge. There is no distinct disk-like structure or prominent spiral arms visible. The isophotes appear generally regular and elliptical, with a slight elongation suggesting an E4-E6 morphological type. There is little evidence of significant dust lanes or recent star formation activity. The overall morphology indicates a relatively undisturbed system that is likely a massive galaxy, potentially with a supermassive black hole at its center.
