The galaxy appears as a relatively small, edge-on disc galaxy. It exhibits a bright central bulge region which gradually fades into a thinner, elongated disc. This disc is not perfectly smooth; there is evidence of some structural features, and some irregularities within the plane. There is no obvious spiral arm structure, but the disc is not uniformly colored, and a few regions seem more prominent. There is a slight color gradient from the bulge outwards, with the bulge appearing whiter and the outer disc showing hints of bluer hues, possibly indicative of younger stellar populations. There is a hint of some interaction but it is not certain, and the possibility of an artifact is also probable. Overall, the galaxy presents as a moderately inclined system.
