The galaxy presents as a slightly elongated, disk-like structure. The central region exhibits a high concentration of luminosity, appearing nearly spherical and intensely bright with a yellowish hue. The surrounding disk shows a more diffuse luminosity, with hints of spiral arm structure, indicated by faint bluish regions suggestive of recent star formation. Redder regions are also present, possibly indicative of older stellar populations or dust lanes. The overall form appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The galaxy possesses a prominent bulge component, potentially indicating a significant population of older stars.
