The galaxy presents as a lenticular or possibly a highly inclined spiral system at a considerable distance. It has a distinctly elongated morphology, exhibiting a cigar-like shape. The central bulge appears relatively smooth and uniform in color, with no obvious signs of active galactic nuclei activity or significant dust lane obscuration. A faint, diffuse disk component may be present, but it is poorly defined. There is a suggestion of a very subtle spiral structure within the disk, but resolution limitations hinder a definitive assessment. The galaxy appears largely undisturbed, with no pronounced tidal features or evidence of recent major merger events. Color gradients suggest the presence of an older stellar population, although a small amount of ongoing star formation may be occurring within the disk region.
