The galaxy presents as a fairly elliptical structure, with a notably bright central bulge that appears to be composed of older stellar populations, indicated by the yellow-orange hue. The overall light distribution suggests a relatively smooth profile, lacking prominent spiral arms or significant dust lanes. The outer regions of the galaxy exhibit a fainter, bluer tint, potentially indicating the presence of younger stars in the disk component. The ellipticity suggests that it is most likely an elliptical or lenticular galaxy. There appears to be no significant ongoing merging activity or major disturbances in its morphology.
