The galaxy presents as an edge-on spiral, exhibiting a prominent dust lane that bisects the galaxy along its major axis. The central bulge appears bright and somewhat elongated, with a concentrated core. The disk component displays a complex morphology with varying degrees of luminosity and potentially disrupted features, suggesting possible interactions or internal disturbances. Overall the galaxy appears to have low star formation. The disk shows a distinct color gradient, the bluer areas likely indicating regions of more recent star formation, contrasting with the redder hues associated with older stellar populations within the bulge. The general luminosity indicates it is a fairly large galaxy.
