The galaxy presents as a centrally concentrated elliptical or lenticular galaxy, exhibiting a smooth, largely featureless morphology. The core displays a yellowish-red hue, potentially indicative of an older stellar population. A more diffuse, greenish halo surrounds the core, possibly resulting from faint, lower-surface-brightness emission. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or recent merger events. The shape is consistent with a near-circular or slightly elliptical distribution. The apparent lack of significant dust lanes or spiral arm structures supports the classification as an early-type galaxy with ongoing, but moderate, star formation.
