The galaxy appears as a moderately bright, elongated structure. It exhibits a smooth, centrally concentrated morphology. The central region displays a yellowish-white hue, potentially indicating an older stellar population. Fainter, bluish regions extend outwards from the central area along the major axis, suggesting the presence of younger stars and possible ongoing star formation. There is a subtle asymmetry in the distribution of the bluer light, with slightly more concentrated light on the right side of the galaxy. Overall, the galaxy presents a relatively undisturbed appearance, with no obvious signs of major mergers or tidal distortions.
