This galaxy exhibits a flattened, elongated morphology, suggestive of a disk galaxy viewed at a high inclination angle. A prominent central bulge dominates the core region, displaying a smooth, concentrated light distribution with a yellowish-white hue. The disk component appears relatively smooth and featureless, with subtle color gradients extending outwards from the bulge. The overall color profile indicates a galaxy with an aging stellar population and a lower rate of current star formation. Evidence of spiral arm structure is not apparent, either due to image resolution or the galaxy's intrinsic morphology. The galaxy displays a cigar shape in the sky. The galaxy does not seem to be undergoing a major merger, but may have some minor disturbances.
