This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The light distribution suggests an elliptical or lenticular type. The galaxy's overall shape appears to be somewhat elongated, deviating slightly from perfect circularity. There is a hint of disk-like structure, although it is not prominently defined. There are no major disturbances or prominent tidal features visible, implying that it is not currently undergoing a major merger. A subtle color gradient is observed, with the central region appearing more yellow-white, potentially indicative of an older stellar population. The outer regions are slightly bluer, which could point to some ongoing, but low level, star formation activity. Overall, the galaxy appears relatively quiescent.
