The galaxy presents as a relatively smooth, elliptical-like structure, although not perfectly round, with a hint of a disk morphology. It exhibits a concentrated central bulge with a strong yellow/orange color, suggestive of an older stellar population dominated by evolved stars. This central region appears to gradually fade into the outer regions of the galaxy. There is a small sign of minor disturbance in the morphology but overall the galaxy appears quite ordinary. The absence of distinct spiral arms or prominent dust lanes supports the classification as an elliptical or lenticular galaxy, where star formation is either minimal or has largely ceased.
