The galaxy presents as a relatively smooth, amorphous structure. It exhibits a somewhat elliptical morphology, deviating from a perfectly circular shape. There is a slight hint of a possible disk structure. The galaxy has a noticeable color gradient, with the central region appearing more yellow in hue, possibly indicating a greater concentration of older stellar populations, compared to the outer regions. The galaxy's light profile appears smooth, indicative of a potentially more evolved system. There seems to be an active region with a slightly bluer tint. There is no apparent spiral arm structure or dust lane presence. Possible minor disturbances from a past or ongoing interaction is not ruled out. 
