The galaxy presents as a lenticular or possibly an edge-on spiral galaxy given its elongated, cigar-like shape. The light distribution appears relatively smooth, suggesting an older stellar population. The galaxy exhibits a subtle color gradient along its major axis, with the central bulge appearing slightly redder than the outer regions of the disk. There's no evidence of prominent spiral arms, strong dust lanes, or significant star-forming regions visible. This galaxy does not show any signs of interactions or disturbances from other galaxies. It is likely an isolated galaxy that has undergone relatively quiescent evolution.
