The galaxy appears to be a spiral galaxy with a prominent, though not overly large, central bulge. Spiral arms are clearly visible, extending outward from the core. These arms exhibit a patchy texture, potentially indicative of active star formation regions. The galaxy displays a bluish hue in its outer regions, consistent with younger stellar populations, particularly within the spiral arms. The central bulge exhibits a more yellowish tint suggesting an older stellar population. While there is a clear spiral structure, it appears somewhat flocculent rather than grand design, lacking well-defined, continuous arms. The overall symmetry appears relatively undisturbed, with no obvious signs of major mergers or strong tidal interactions. Some minor distortions or irregularities in the outer regions cannot be ruled out, but the galaxy maintains a generally settled and organized morphology. There is a faint disk around the bulge. The bar is very faint, but seems to extend horizontally in the image.
