The galaxy presents a generally smooth appearance, with a noticeable concentration of light towards the center. The light distribution suggests a spheroidal shape, being fairly round. The central region exhibits a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions show a bluer tint, which could point towards more recent star formation activity. There is some slight indication of possible minor disturbances in the outer disk, but a distinct disk structure is not readily apparent. Based on color and light profile, it could be a galaxy in transition between a spiral and elliptical morphology.
