The galaxy presents as a centrally concentrated, smooth system. It exhibits an elliptical morphology, appearing somewhat elongated, though approaching a more circular shape. The core is luminous and characterized by a yellow-white hue, suggesting an older stellar population. A fainter, more diffuse halo extends outwards from the core, displaying a reddish tint. The smooth light distribution indicates a lack of prominent spiral arms or strong dust lanes. There is little evidence of ongoing major mergers, although the galaxy may be exhibiting minor gravitational disturbances based on some irregularities within the halo structure. Overall, the galaxy appears to be a relatively massive system with a suppressed rate of star formation.
