The galaxy presents as a somewhat elongated, cigar-shaped system. It exhibits a prominent central bulge that appears relatively smooth and concentrated. Faint and loosely defined spiral arm structures are present, but not clearly delineated. The color profile suggests a dominant population of older stars within the bulge, while some bluer regions hinting at ongoing star formation may be present within the disk. There is some evidence of minor disturbances within the galaxy structure, but it does not seem to be undergoing a major merger.
