The galaxy presents as a smooth, elongated structure, approximately 5.5 kpc in radius based on estimated half light radius. Its shape is distinctly prolate, appearing somewhat cigar-shaped. The luminosity profile appears relatively uniform, lacking prominent spiral arms or a bright, concentrated nucleus. The color gradient suggests a centrally concentrated population of older stars, giving off a yellowish hue in the center. The outer regions appear bluer, possibly indicating more recent, ongoing star formation. The overall smooth appearance indicates a galaxy that has either undergone significant dynamical relaxation, or has not experienced a recent major merger. It seems to only have minor disturbances. The lack of substantial substructure is notable.
