The galaxy presents a primarily smooth and concentrated morphology. It exhibits a bright, elliptical core that dominates the overall structure. The light profile suggests a central bulge with a gradual decrease in luminosity extending outward. There is little evidence of distinct spiral arms or significant dust lanes. The color appears to be relatively uniform throughout the galaxy, exhibiting a yellowish-orange hue, suggesting a population of older stars. There may be some minor asymmetry or disturbance in the outer regions, but the overall structure appears largely undisturbed. The lack of strong blue color indicates a low star formation rate.
