This galaxy presents as a spiral galaxy, though its angle relative to our line of sight makes it difficult to fully discern its arm structure. The central bulge is prominent and appears moderately sized, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter spiral arms extend outward from the bulge; these arms show clumpy regions of bluer light, indicating regions of more recent star formation. The arms exhibit moderate winding. There are some faint areas of disturbance, perhaps due to tidal interaction, but likely not. The disk appears largely intact and well-defined. 
