The galaxy presents as a centrally concentrated, elliptical-like structure. The core region exhibits a higher luminosity, gradually decreasing toward the outer edges, which appear rather diffuse. It displays a smooth morphology, with no apparent spiral arm structures or prominent dust lanes. There is only a slight indication of a disk-like shape. The color gradient ranges from a yellow or orange hue in the core to a slightly bluer tone in the extended halo, possibly indicating older stellar populations in the central region. The galaxy appears relatively isolated, without significant tidal distortions or signs of recent mergers. Overall, the morphology indicates an evolved system, likely with diminished star formation activity.
