The galaxy presents as a relatively smooth, somewhat elongated structure. Its overall color profile suggests a dominance of older stellar populations, with a central bulge exhibiting a yellowish-white hue. Fainter, bluer regions can be seen in what is likely a disk, indicating regions of ongoing star formation. The galaxy appears to be a disk galaxy that is somewhere between round and cigar-shaped when looking at it edge-on. There are no signs of major mergers or significant disturbances in the image, but there might be very minor disturbances.