The galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology. A prominent central bulge is visible, displaying a yellowish hue, potentially indicative of an older stellar population. The disk appears thinner with a bluish tinge, potentially indicating a younger stellar population and ongoing star formation. Evidence suggests the presence of faint dust lanes within the galactic disk. There are subtle hints of spiral arm structure visible in the outer regions of the disk. The disk exhibits a smooth, streamlined appearance, with no major disturbances or signs of a recent merger. The galaxy appears relatively isolated, with no other large galaxies nearby.
