The galaxy presents an elliptical morphology, characterized by a smooth and centralized light distribution, displaying a dominant yellowish core with a red halo. The primary structure exhibits a high degree of symmetry with no apparent spiral arms. No significant dust lanes or patches are observed within the galactic disk, indicating a relatively quiescent star formation rate. The overall light profile suggests an older stellar population with fewer hot, young stars contributing to the blue light. There is a possible minor disturbance, but this may be a result of resolution. The galaxy does not present any apparent merger events.