The galaxy presents as a centrally concentrated object, approximately round in appearance. It exhibits a smooth morphology, with a notable lack of distinct spiral arms or other features. The light distribution suggests an elliptical or lenticular classification. 

The galaxy appears to be composed primarily of older stellar populations, indicated by the redder color in the central region, transitioning to slightly bluer hues in the outer regions. This color gradient likely reflects ongoing, though potentially diminished, star formation activity. The overall apparent magnitude suggests this is a moderately luminous galaxy, and its apparent size suggests it is relatively compact. There is no evidence of significant tidal distortions or ongoing major merger activity, although subtle disturbances cannot be ruled out based on this image alone.
