The galaxy presents as a flattened, disk-like structure, oriented nearly edge-on relative to the observer's line of sight. A central bulge is visible, appearing bright and relatively smooth in texture. The disk component shows some indications of substructure, potentially spiral arms or dust lanes, but is mostly uniform in color and lacks distinct knots of star formation. The light distribution appears asymmetrical, potentially indicating a mild gravitational interaction or recent accretion event. Color gradients suggest a transition from bluer regions near the center to redder hues towards the periphery. Overall, this galaxy exhibits characteristics of a late-type spiral or lenticular galaxy seen at a high inclination. Some irregularities are present that may be the results of minor disturbances or a potential merger.
