The galaxy presents as a late-type spiral system viewed nearly edge-on. A prominent central bulge exhibits a yellowish hue, suggestive of an older stellar population. A flattened disk extends outwards from the bulge, displaying a reddish coloration at the edges indicating dust extinction. The disk appears relatively smooth with no obvious distinct spiral arm structures.  A slight warping of the disk is suspected.  A faint blue haze is also visible, indicating recent or ongoing star formation.