The galaxy presents a somewhat elongated, cigar-shaped morphology. A concentrated, bright central bulge dominates the galaxy's core. Extending outward from the bulge, fainter and more diffuse disk-like structures are observed, though distinct spiral arm features are not readily apparent. The overall color profile suggests a significant population of older stars, particularly within the central bulge, which exhibits a yellowish-golden hue. The disk regions appear slightly bluer, hinting at ongoing, although potentially low, levels of star formation activity. There is no obvious evidence of major mergers or significant tidal disturbances in this image, but there is a slight asymmetrical bulge in the center, along with minor disturbances within the disk. The galaxy appears relatively smooth in texture, implying a well-mixed stellar population without prominent knots of star formation.
