The galaxy presents as a relatively smooth, elongated structure, appearing cigar-shaped in its morphology. The central region exhibits a brighter, more concentrated luminosity, indicating a likely bulge component. Moving outward from the center, the luminosity gradually decreases. There is a subtle color gradient, where the central region is dominated by warmer colors, and the outer regions are more blue. There is no visual evidence of significant spiral arm structures or prominent dust lanes; however, there may be a sign of minor disturbance. The galaxy does not display characteristics of a major ongoing merger, though a minor disturbance may be present. It presents an elliptical galaxy.
