The galaxy exhibits a roughly elliptical morphology. A bright, concentrated central bulge dominates the galaxy's core, emanating a strong, almost point-like source of light. Surrounding the bulge is a more diffuse disk component. The disk appears relatively smooth, with a faint blue-green hue suggestive of ongoing star formation. There is a slight indication of minor disturbances or asymmetry within the outer regions of the disk. A faint, extended halo may also be present, surrounding the main body of the galaxy. The galaxy's overall color gradient indicates a likely transition from older stellar populations in the central bulge to younger, bluer stars within the outer disk regions.
