The galaxy presents a generally smooth morphology, appearing as a slightly elliptical, unresolved object. The primary body exhibits a diffuse, yellowish hue, indicative of a population of older stars. There is a faint suggestion of a disk-like structure. A minor degree of disturbance is seen, potentially from a past minor interaction or internal instability. Overall, the galaxy appears relatively undisturbed and mature, with limited evidence of ongoing major star formation. 
