The galaxy exhibits a generally smooth, elliptical morphology. The central region appears brighter and more concentrated, indicating a significant bulge component. There is a noticeable radial color gradient, transitioning from a yellowish-white core to a more reddish outer halo. No distinct spiral arms or prominent dust lanes are discernible in the image. There is some subtle asymmetry in the outer isophotes, with hints of extended light on one side, which could indicate a possible minor tidal disturbance or interaction. The galaxy appears relatively isolated, with no obvious signs of a major merger event in progress. The overall color suggests a moderate population of older stars.