The galaxy exhibits an elliptical morphology, appearing as a centrally concentrated spheroid of light. The core region displays a yellowish-orange hue, potentially indicative of an older stellar population and lower levels of ongoing star formation within this area. Moving outwards from the central bulge, there appears to be a transition to a slightly bluer color, which may indicate younger stars. There are no distinct spiral arms or bar features visible. Overall, the galaxy appears relatively undisturbed. There is no evidence of strong tidal features, major mergers, or significant dust lanes. The smoothness of the light distribution suggests that the galaxy is well-mixed and possibly a product of past mergers or interactions.
