The galaxy exhibits a flattened, elongated morphology, appearing cigar-shaped from our perspective. A central bulge is visible, displaying a concentrated, yellowish hue, indicating an older stellar population dominating the core. The disk appears relatively smooth and shows a bluish tinge, suggesting ongoing star formation. The galaxy does not exhibit prominent spiral arm structures. Overall, the galaxy appears relatively undisturbed, with no major signs of mergers or tidal disruptions.
