The galaxy presents as an edge-on spiral, exhibiting a distinct flattened disk. A prominent central bulge appears yellowish, possibly indicating an older stellar population and/or dust obscuration. The disk shows a bluish hue along its edges, suggesting the presence of younger, hotter stars formed more recently in these regions. There is no obvious bar structure or signs of active galactic nuclei emission. The disk seems fairly smooth, but without higher resolution it is hard to determine distinct dust lanes or spiral arm structures. There is no evidence for recent major mergers or tidal disturbances in the galaxy's overall morphology. The galaxy is approximately 14 kiloparsecs in diameter.