This galaxy appears to be an elliptical, lenticular, or possibly a spiral galaxy viewed at an angle. The galaxy exhibits a smooth, centrally concentrated bulge that dominates the overall light profile, suggesting a large stellar mass. There appears to be a flattened disk component with little visible structure, such as spiral arms. The color gradient transitions from a yellowish-orange central region to a faint blue/greenish hue toward the outer edges. The lack of clear spiral arm structures and the dominant central bulge suggest that the star formation is most likely occurring within the disk and is very low. The overall shape indicates the galaxy is not perfectly spherical, and it is not currently undergoing a major merger. There may be a very minor disturbance in the galactic structure, but the overall impression is of a relatively settled, evolving galaxy.
