This galaxy appears to be a spiral galaxy, likely seen at an oblique angle. There is a bright, yellowish central bulge that dominates the visual structure, suggesting an older stellar population concentrated in the core. Fainter, bluish regions extend outwards from the bulge, potentially indicating the presence of younger stars and ongoing star formation within the galactic disk. Although no defined spiral arm structure is readily apparent in this image, the disk features exhibit subtle irregularities and disturbances. There is a slight asymmetry to the distribution of light across the disk. Based on its smooth appearance, the galaxy does not appear to be undergoing any major merging events, with only minor distortions present.
