The galaxy presents a disk-like morphology, viewed at a near edge-on angle. There is a noticeable central bulge, appearing smooth and concentrated, with a yellowish hue. The disk itself exhibits a bluish tint, suggesting the presence of younger stellar populations and ongoing star formation. There are no obvious spiral arm structures readily discernible, likely due to the viewing angle, though some subtle variations in brightness within the disk may indicate underlying structure. The galaxy appears relatively isolated, with no apparent signs of tidal interactions or major mergers with other galaxies in its immediate vicinity. Overall, the galaxy presents a well-defined and relatively undisturbed structure.
