The galaxy presents as a relatively small, edge-on spiral with a somewhat elongated profile. It exhibits a noticeable central bulge. The disk component is primarily blue, indicative of ongoing star formation. There is an absence of clearly defined spiral arm structures, suggesting the galaxy is either relatively old, has experienced recent tidal disturbances, or is a flocculent spiral. The disk appears relatively thin. The color gradient suggests there is little to no dust extinction between the observer and the stars within. The outer regions of the galaxy show a fainter, more diffuse glow, possibly indicating the presence of a stellar halo or the outer reaches of the galactic disk. The galaxy's overall structure appears relatively undisturbed, with no obvious signs of a major merger event in its recent past.
