The galaxy presents as a relatively smooth, elliptical-like structure. Its light is concentrated toward the center, with a gradual decrease in intensity outward. The core region exhibits a yellowish-white hue, suggesting a population of older stars. Fainter, bluer regions are observable in the outer areas, hinting at the presence of younger stars and regions of ongoing star formation. The overall shape is neither perfectly round nor highly elongated, appearing somewhere in-between. There's some indication of minor structural disturbance. Possible interactions might be influencing its morphology.
