The galaxy presents as a generally smooth, centrally concentrated object. There is a slight elongation, but no distinct spiral arm structure is discernible. Color gradients suggest some variation in stellar populations or dust content across the galaxy, with a generally redder core and slightly bluer outer regions. There are no apparent signs of significant tidal disturbances or ongoing major mergers, though a minor disturbance cannot be ruled out. The galaxy appears relatively undisturbed, with a smooth overall structure.
