This galaxy presents as a relatively smooth, elongated structure. The central region exhibits a brighter, more concentrated luminosity, suggestive of a galactic bulge. The overall color profile suggests a combination of older stellar populations, indicated by the reddish hue in the central bulge, and a younger, star-forming population present in the surrounding disk, marked by greenish and bluer tints. No prominent spiral arms or bar structures are immediately visible. The disk appears relatively undisturbed, without signs of significant tidal interactions or major mergers, although a minor disturbance cannot be ruled out. The morphology appears to be somewhere between round and cigar shaped, with the bulge dominating its overall form.
