The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual falloff in surface brightness towards the outer regions. Color gradients suggest a relatively homogenous stellar population, with a slightly bluer hue in the central region, possibly indicating a low level of ongoing star formation. The galaxy exhibits no obvious spiral arm structures or significant dust lanes, consistent with an early-type classification. There are minor irregularities or distortions that might indicate a recent or ongoing interaction. The galaxy is not perfectly spherical, but also not particularly elongated. The overall appearance is indicative of a mature system.
