The galaxy appears to be a relatively compact, early-type system, possibly an elliptical or lenticular galaxy. It exhibits a centrally concentrated luminosity profile, with a bright, unresolved core that likely hosts a supermassive black hole. The overall color is slightly redder, suggesting an older stellar population with a lower rate of ongoing star formation. The galaxy's morphology appears relatively smooth, lacking prominent spiral arms or significant dust lanes. There is a slight indication of a disk-like structure but further information is required to verify this. The shape is tending to round, rather than oblong. There is a chance of minor disturbances.
