The galaxy presents as a flattened elliptical shape, viewed at a significant angle relative to its plane. The central region exhibits a high degree of concentration of light, suggesting a substantial bulge component. Moving outward from the core, the intensity of the light decreases gradually into a fainter disk. Faint traces of spiral arm structures may be present, appearing as subtle deviations from the smooth disk. The galaxy displays a color gradient, transitioning from yellow-ish to a blue-ish hue from the center to the edges, indicating a younger stellar population in the outer regions. Overall, the galaxy appears as a relatively smooth and evolved system with subtle signs of more recent star formation. There is no obvious evidence of major merger activity.