The galaxy presents as an edge-on spiral with a prominent bulge. The bulge region exhibits a concentration of older stars, indicated by the yellowish-red hue. Fainter, bluish dust lanes are present, concentrated along the equatorial plane, obscuring the light from regions behind them. The galaxy shows an elliptical shape, with a flattened disk extending outward from the central bulge. There is no evidence of major mergers or strong tidal features, suggesting it is relatively undisturbed. The overall light distribution appears smooth, with no indications of distinct star-forming regions.
