The galaxy presents a generally smooth appearance, with a slight elongation along one axis. The core region displays a concentrated luminosity, suggesting a high density of stars and potentially a central supermassive black hole. There is a discernible color gradient, with the core exhibiting a yellowish hue that transitions towards a bluer tinge in the outer regions. This color difference may indicate variations in stellar populations, with older stars concentrated towards the center and younger, hotter stars present in more distal areas. A faint extension can be seen on one side of the galaxy, which could be either an artifact of a tidal interaction or the beginnings of a spiral arm structure. Further analysis is needed to resolve the nature of the observed extension and other possible substructures within the galaxy.
