The galaxy presents as a relatively smooth, elliptical object. The core displays a concentrated, bright luminosity, potentially indicative of a substantial central mass concentration, possibly a supermassive black hole. The light gradually diffuses outward, exhibiting a lack of prominent spiral arm structures or distinct star-forming regions. There is a color gradient present, with the central region appearing more yellow/orange, suggesting a population of older, redder stars, while the outer regions tend towards a slightly bluer hue. The galaxy is somewhat rounded in shape, and it shows no obvious signs of significant disturbances or ongoing mergers. Based on the smooth profile and the observed color gradient, star formation is likely suppressed.