The galaxy presents as a somewhat elliptical structure, with a smooth, diffuse appearance. A central bulge is discernable, exhibiting a yellowish-orange hue, suggesting a population of older stars. Fainter, bluish light surrounds the central bulge, possibly indicative of more recent star formation within a disk-like component. The galaxy appears relatively undisturbed, without significant tidal features or strong asymmetries. The overall color gradient indicates a transition from older stellar populations in the center to potentially younger populations in the outer regions. There is little evidence of spiral arm structure, and the light distribution is concentrated towards the center.
