The galaxy presents as a relatively faint, elongated object. It appears to be an edge-on spiral galaxy, exhibiting a well-defined, flattened disk structure. A prominent central bulge is evident, displaying a yellowish hue, suggesting an older stellar population. The outer regions of the disk show a bluer tint, possibly indicative of younger, hotter stars and ongoing star formation. The galaxy seems relatively undisturbed, with no major signs of recent mergers or tidal interactions. The disk displays a high degree of symmetry. The estimated physical size of the galaxy indicates it to be of moderate scale.
