The galaxy presents as a highly inclined, almost edge-on disk galaxy. A prominent dust lane bisects the galaxy along its major axis, obscuring the central regions. The bulge appears relatively small and indistinct. The disk exhibits a faint blue hue at its outer edges, possibly indicating regions of ongoing star formation. The overall color suggests a mix of stellar populations, with older, redder stars concentrated towards the bulge and younger, bluer stars populating the disk. There is no visual evidence of a major merger or strong tidal interaction, although some minor asymmetry might be present. The galaxy's light distribution appears relatively smooth, with a slight central concentration.
