The galaxy presents as a primarily elliptical morphology with a smooth, concentrated light profile. The core exhibits a yellowish-white hue, suggestive of an older stellar population. There is a slight elongation observed, with its largest radius estimated at approximately 4 kpc. The galaxy is characterized by a minimal presence of defined features, indicating a low rate of ongoing star formation. A small disturbed section can be noted at the very edge of the galaxy. The overall impression is that of a relatively evolved galaxy with a substantial stellar mass.
