The observed galaxy presents as an edge-on spiral system. A prominent central bulge is visible, exhibiting a smooth, concentrated morphology with a yellowish hue, indicative of an older stellar population. A thin, extended disk extends outwards from the bulge, displaying a fainter, bluer color profile suggestive of ongoing star formation. The disk appears relatively undisturbed, with no clear signs of major tidal interactions or mergers. There is an interesting, reddish feature at the outer edge of one side of the disk. This may be due to a star forming region, or some other internal activity of the galaxy.
