The galaxy appears as a centrally concentrated object with a moderately elliptical shape. It presents a smooth, relatively featureless morphology, with no apparent spiral arms or distinct dust lanes. The central region exhibits a higher surface brightness, suggesting a prominent galactic bulge. The color profile across the galaxy appears relatively uniform, with a slight trend toward bluer hues in the outer regions and a whiter core. This might suggest older stellar populations dominate the core while there may be some recent star formation in the outer regions. There is no apparent evidence of any major ongoing merger activity or significant tidal distortions, although a subtle asymmetry suggests possible minor interaction. The galaxy's overall light distribution indicates it could be a disk galaxy or a lenticular galaxy.
