The galaxy presents as a flattened, elongated structure, highly inclined to our line of sight. It exhibits a clear disk-like morphology, viewed nearly edge-on. The central bulge appears prominent and exhibits a somewhat rounded shape. There is evidence of internal structure, with slight indications of dust lanes or spiral arm fragments visible within the disk. The disk appears smooth and has subtle irregularities. The overall color of the galaxy seems to be biased towards redder hues, suggesting an older stellar population. There is no visible evidence of a major ongoing merger or significant tidal disruption. It appears to be a relatively isolated system.
