The galaxy presents as a flattened, disk-shaped structure, viewed at a high inclination relative to our line of sight. Its appearance suggests it may be an edge-on or nearly edge-on spiral or lenticular galaxy. The light distribution indicates a central bulge region that is not very prominent, with a relatively smooth brightness profile. The disk component exhibits some evidence of internal structure, possibly spiral arms, though these features are not sharply defined. The galaxy's light is noticeably bluer than expected, especially at the edges, which is indicative of ongoing star formation activity. There may be evidence of minor gravitational disturbance, but this is difficult to tell without further data.
