The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated core region transitions gradually into a fainter, more diffuse halo. The core exhibits a yellowish-white color, suggesting a population of older stars. Moving outward, the halo displays a subtle bluish tint, potentially indicative of younger stars. A slight disturbance is visible in the outer regions. There may be some minor tidal features present, perhaps resulting from a past interaction or ongoing minor merger event. Overall, the galaxy appears to be relatively massive and in a late stage of its evolution, with a suppressed star formation rate. The galaxy has an estimated size of about 5 kpc across.
