The galaxy appears to be an elliptical or lenticular type, characterized by a relatively smooth and centralized light distribution. There is a lack of distinct spiral arm structures, and minimal dust lane presence is observed. The galaxy appears to be intermediate in roundness, leaning towards an in between shape. There is no evidence of ongoing or recent major merger events, although subtle disturbances are possibly present within the galaxy. The galaxy has a strong central bulge, with a possible active galactic nucleus emitting intensely. Star formation rate is low. The galaxy presents a red hue indicating a population dominated by older, redder stars. Overall, it appears to be a relatively quiescent system.
