This galaxy exhibits a generally smooth morphology, suggesting an elliptical or lenticular classification. The central region displays a concentrated, bright core, surrounded by a more diffuse halo. The overall color appears to be redder or yellower, indicative of an older stellar population with relatively low recent star formation. There is a slight asymmetry or subtle feature that hints at a possible past interaction or minor disturbance, or it could be related to internal dust obscuration. The galaxy is moderately large in size and has a high stellar mass.
