The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge with a radial color gradient, transitioning from a blue-white core to a slightly redder outer halo. The isophotes appear generally round, though a subtle elongation is detectable. There is a faint, diffuse structure extending from the main body, potentially indicating a minor tidal disturbance or interaction. The overall color suggests a moderate amount of star formation activity, with a significant population of older stars contributing to the redder hue. There is some evidence of possible dust lanes within the halo, although it appears largely featureless.
