The galaxy presents as a centrally concentrated object with a smooth overall appearance. The light distribution is centrally peaked with a noticeable radial falloff. The core region emits strongly in yellow and appears quite dense. Moving outward, the galaxy exhibits a more diffuse yellow glow, fading into redder hues at the periphery. There is little evidence of spiral arm structures or significant dust lanes. The galaxy appears to be relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. The morphology is generally elliptical or lenticular, and fairly round. There is a slight hint of a disk-like structure, but the smooth luminosity profile dominates. Overall, the galaxy appears to be a relatively quiescent system, perhaps transitioning away from a star-forming phase.
