The galaxy presents a largely smooth, elliptical morphology. It appears nearly round in shape, showing minimal apparent deviation from a circular form. The central region displays a high concentration of light, gradually decreasing in intensity towards the outer edges. The color profile suggests a dominant population of older stars, with a yellowish hue in the core transitioning to a slightly bluer outer halo. There is a possible, though subtle, indication of minor disturbance or interaction within the galaxy, though no clear merging features are visible. The overall structure points towards a relatively quiescent system with a moderate stellar mass.
