The galaxy presents as a centrally concentrated, relatively smooth object with a dominant spheroidal morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color transitions to a slightly redder shade, and the surface brightness diminishes. There is minimal evidence of spiral arm structure or significant dust lanes. The overall shape is roughly circular. The galaxy appears mostly undisturbed, with no obvious signs of major mergers or tidal interactions. There is slight evidence of redder emissions on the edges of the galaxy.
