The galaxy presents as an edge-on spiral or lenticular galaxy, exhibiting a notable disk structure oriented almost perfectly along our line of sight. There is likely an actively star-forming region within the galaxy, and it also possesses a luminous central bulge, the color suggests an older stellar population in this region, possibly with a supermassive black hole at the center. The disk appears relatively smooth, without prominent, well-defined spiral arms. The overall morphology suggests a relatively undisturbed system, with no clear signs of ongoing major mergers or tidal interactions. From the color, there seems to be a significant amount of dust within the plane of the disk, attenuating and reddening the light from stars behind it.
