The galaxy presents as a relatively small, elongated structure, observed edge-on. There's a notable central bulge that appears largely spheroidal. The disk component appears thin and exhibits a distinct color gradient, transitioning from a yellow-orange hue in the central regions to a fainter, slightly bluer tone towards the outer edges. This may be due to varying stellar populations and dust distribution within the galaxy, with younger stars towards the edge of the galaxy and older stars toward the center. No significant signs of strong tidal interactions or major morphological disturbances are apparent.
