The galaxy presents as a moderately inclined, elongated structure. Its morphology is indicative of a disk galaxy, potentially an early-type spiral or a lenticular galaxy, given the relatively smooth appearance and subtle colour gradient. The central bulge region exhibits a yellowish-white hue, suggesting an older stellar population. The disk shows hints of bluer colours, particularly towards the outer edges, possibly indicating regions of ongoing, but diminished, star formation. There is a lack of distinct spiral arm structure and bright HII regions. The galaxy appears relatively undisturbed with no apparent signs of recent major mergers or tidal interactions. The disk appears to be approximately twice as long as it is wide, with no major warps or distortions. Overall, it appears to be a fairly compact galaxy.
