This galaxy appears to be a spiral galaxy, viewed at a significant angle, close to edge-on. A prominent central bulge is visible, exhibiting a yellowish-orange hue, indicative of an older stellar population. The spiral arms are faintly discernible as bluish-white bands extending from the bulge, suggesting ongoing star formation. Patches of darker material, possibly dust lanes, can be observed within the spiral arms. The overall structure appears somewhat disturbed or irregular, potentially due to past interactions or internal processes. There is faint, diffuse light extending beyond the main body of the galaxy, forming a halo. A possible, small companion or merging object may be influencing the structure on the left side.
