This galaxy presents a generally elliptical morphology, though subtle features suggest a more complex underlying structure. The central region exhibits high luminosity and a smooth texture, characteristic of a prominent bulge. Moving outward from the core, there's a gradual decrease in surface brightness, indicating the presence of an extended disk component. Within this disk, hints of spiral arm structure can be discerned, although the arms are not sharply defined and appear somewhat flocculent. The color profile shifts from a predominantly white or yellow hue in the center to a slightly bluer tint in the outer regions, which may indicate the presence of younger stellar populations in the disk. The overall appearance suggests that this galaxy is not undergoing a major merger or strong tidal interaction, but there might be minor disturbances or asymmetries in the outer disk. 
