The galaxy presents as a moderately bright, centrally concentrated object. It exhibits a generally elliptical morphology, displaying a degree of elongation. The central region appears smooth and featureless, with a bright, yellow hue, likely indicative of an older stellar population. Progressing outward from the core, the color gradually shifts towards a bluer and fainter periphery. There is little evidence of distinct spiral arm structure, and the overall structure appears relatively undisturbed, though some faint irregularity to one side indicates a possibility of a minor disturbance event. The galaxy's spatial extent is substantial, suggesting a reasonably large physical size.
