The galaxy presents a moderately luminous appearance. Morphologically, it exhibits a somewhat elliptical shape, appearing more elongated than circular, but not extremely so. The central region displays a brighter, more concentrated light profile, indicating a possible bulge. Diffuse, fainter extensions of light emanate from the central region, suggesting the presence of a disk component, possibly with faint spiral arms or simply a more amorphous distribution of stars and gas. The color gradient seems to show a shift from bluer outer regions to redder inner regions, possibly indicating older stellar populations are concentrated in the center. There is some evidence of possible disturbance or interaction, perhaps a tidal tail or distortion in the shape, hinting at a past or ongoing merger event. A smaller, more compact galaxy appears nearby, and it may be interacting with the larger galaxy. The galaxy displays some features which are consistent with relatively low star formation rate.
