The galaxy presents as a cigar-shaped, elongated structure. It exhibits a relatively smooth morphology, though there is some subtle, irregular structure in the disk. The main body of the galaxy displays a yellowish-white hue that transitions into a more reddish hue towards one end, suggesting possible differences in stellar populations or dust content. There is a bluer, less defined area, at the opposite end, hinting at regions of ongoing star formation. Based on the colour and morphology, it is potentially an edge-on disk galaxy, possibly a lenticular galaxy, with some evidence of recent or ongoing star formation. It appears relatively isolated, with no obvious signs of a major ongoing merger, but there is subtle warping or disturbances in the outer regions, suggestive of minor gravitational interaction or internal dynamics.
