This galaxy presents as a spiral galaxy viewed edge-on. A prominent, centrally concentrated bulge dominates the light profile, displaying a yellowish hue, suggestive of an older stellar population. The disk appears flattened and extended, with a more diffuse, fainter luminosity compared to the bulge. There is a clear dust lane visible bisecting the disk horizontally. The disk shows possible signs of faint spiral arm structures, hinting at ongoing star formation. Overall, the galaxy displays a smooth and regular morphology without any major disturbances, suggestive of a relatively isolated system. The lack of blue colour suggests the galaxy is either a red spiral or has a low rate of star formation. The absence of visible tidal features implies no recent major merger events.