The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated, bright luminosity, transitioning outwards to a less intense halo. Subtle color variations are observed, with the central region appearing more yellow-orange, possibly indicating an older stellar population. Fainter bluish hues are visible in the outer regions of the disk, suggesting the presence of some younger, hotter stars. There's a very slight asymmetry in the shape and light distribution, giving a possible indication of a minor gravitational disturbance or past interaction. Overall, the galaxy appears relatively isolated and well-defined. The scale of the object indicates a substantial mass and a considerable distance. Star formation seems to be happening but at a slow rate.
