The galaxy presents as a flattened, disk-like structure seen at a significant angle. It exhibits a central bulge that appears relatively smooth and concentrated, displaying a yellowish-orange hue. Emanating from the central bulge is a fainter, extended disk component, somewhat elongated and more cigar-shaped than circular. The disk shows hints of internal structure, potentially representing faint spiral arm segments. Overall color suggests a galaxy dominated by an older stellar population, possibly undergoing a moderate level of star formation. There is no obvious strong evidence of significant ongoing merger activity or tidal disturbances.
