This galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. The central region displays a yellowish hue, suggestive of an older stellar population dominated by redder stars. The isophotes appear generally regular, with a slight elongation along a major axis. There's no evidence of prominent spiral arms, dust lanes, or significant star-forming regions. The overall structure appears relatively undisturbed, with no clear signs of recent major mergers or tidal interactions. The smooth light distribution and color gradients are consistent with a galaxy that has largely completed its star formation and is now populated primarily by evolved stars.
