The galaxy presents as a relatively faint, edge-on spiral, exhibiting a prominent dust lane obscuring the galactic center. The dust lane is characterized by a dark, reddish-brown hue and appears relatively smooth, suggesting a significant presence of interstellar dust. Above the dust lane, a distinct disk is visible, exhibiting a bluish-white color profile indicative of a younger stellar population and ongoing star formation. There is a central bulge with a slight yellowish tint, which may indicate the presence of older stars. The overall structure appears somewhat disturbed, possibly due to minor gravitational interactions, although no major merging features are immediately apparent. The galaxy's star formation rate appears to be low.
