The galaxy presents a predominantly smooth morphology, appearing as a slightly elliptical structure. There is a concentration of light towards the galactic center, which gradually diffuses outward. The galaxy exhibits a subtle color gradient, transitioning from a yellowish-white core to a more reddish-tinged outer region. No distinct spiral arms or prominent dust lanes are visible, suggesting it may be a relatively evolved system. There are no obvious signs of ongoing major mergers or significant disturbances within the visible structure. The overall light distribution indicates a spheroidal or elliptical galaxy type.
