The galaxy presents as a single, relatively smooth object with a centrally concentrated brightness profile. The core region exhibits a bright, yellowish hue, suggesting a population of older stars. Progressing outwards from the center, the color shifts slightly towards a greenish tint before transitioning into a diffuse outer halo. The outer regions appear less structured. There is a faint suggestion of asymmetry in the outer halo, possibly indicating minor disturbances to the overall structure. The galaxy displays a generally rounded morphology, lacking prominent spiral arms or a well-defined disk. There is no visual evidence of a major ongoing merger.
