The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless light profile. The central region displays a concentrated luminosity, indicative of a bulge, possibly hosting a supermassive black hole. The color gradient suggests an older stellar population, with a dominant yellow-red hue in the core transitioning to a bluer periphery. There is no evidence of spiral arms or significant dust lanes. The overall structure appears undisturbed, with no signs of recent major mergers or tidal interactions.
