The galaxy presents as a relatively faint, edge-on spiral system. The central bulge appears prominent and exhibits a yellowish-orange hue, suggestive of an older stellar population. A flattened disk structure is visible, extending outwards from the bulge, and is oriented nearly along our line of sight. Within the disk, hints of obscuring dust lanes are subtly present, further indicating its edge-on nature. The outer regions of the disk appear diffuse and less defined, possibly due to lower surface brightness or interactions. There is a slight asymmetry in the outer regions of the disk, potentially indicative of minor tidal disturbances or past interactions, but no obvious signs of major mergers or strong tidal features are apparent. Overall, the galaxy appears to be a quiescent, moderately massive system with a low star formation rate.
