The galaxy presents as a flattened, elliptical morphology. It exhibits a bright, concentrated central bulge, with a gradual decrease in luminosity outwards toward the edges of the galaxy. There appears to be a lack of distinct spiral arm structure, instead showing a smooth, diffuse distribution of light. The color profile suggests a population of older stars, indicated by the predominantly yellowish-white hue, although some blue light is also observed. There may be some dust lanes visible, causing a degree of internal extinction. Overall, the galaxy appears relatively undisturbed and shows no signs of recent major merger events.
