The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's light profile, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The surrounding halo appears more diffuse, fading into the background. The overall structure indicates a system with little to no active spiral arm structure or significant dust lanes. There is no obvious sign of a recent major merger, although there seems to be a very faint, very minor irregularity present. The isophotes appear mostly regular. The galaxy shows a slightly rounded appearance, neither perfectly spherical nor highly elongated. Overall, the galaxy appears consistent with an early-type galaxy that is not actively star-forming.
