This galaxy exhibits a clear disk-like morphology, viewed nearly edge-on from our perspective. The central bulge is prominent and appears to be populated by older stars, indicated by the yellowish-orange hue. The galactic disk displays a bluer color, suggestive of ongoing star formation. There is a slight asymmetry in the disk's light distribution, possibly caused by minor gravitational interactions. No distinct spiral arm structure is visible, likely due to the edge-on viewing angle and the limited image resolution. Overall, the galaxy seems relatively undisturbed, displaying no signs of a major merger event.
