This galaxy presents as a flattened, disk-like structure, likely a spiral or lenticular galaxy observed at an oblique angle, somewhere between face-on and edge-on. There's a noticeable central bulge that appears smooth and concentrated, suggesting an older stellar population in the nucleus. Surrounding the bulge is a more diffuse disk. Faint spiral arm structures may be present within the disk, though they're not sharply defined and somewhat patchy in appearance. There's a hint of blueish color concentrated to some regions within the disk, which could indicate regions of ongoing star formation and the presence of younger, hotter stars. However, the overall color is relatively muted, with a general yellow-white hue, implying a relatively low rate of star formation compared to other spiral galaxies and a substantial population of older stars. There is a possible hint of a dust lane on the lower side of the galaxy. Overall, the galaxy exhibits a morphology suggestive of a disk galaxy undergoing moderate to low levels of star formation. It shows possible signs of disturbance/merging.
