The galaxy presents a generally smooth morphology, with a centrally concentrated brightness profile. The shape appears to be generally round. There is some indication of a disk feature. The galaxy exhibits a color gradient, transitioning from a yellowish core to bluer outer regions. The bluer regions suggest the presence of younger stellar populations and ongoing star formation. There is no clear evidence of tidal features or major mergers, although minor disturbances may be present. The light distribution suggests it is an evolved galaxy. The overall structure indicates a system that is likely undergoing or has undergone a period of significant star formation.
