This galaxy exhibits a predominantly smooth morphology, with a central bulge that appears roughly ellipsoidal in shape. The galaxy displays a subtle disk-like structure, although distinct spiral arms are not readily apparent in the image. Color gradients suggest that the central bulge contains older stellar populations, indicated by the yellow/orange hue, while the outer regions display a bluer tinge, potentially indicative of ongoing or recent star formation. There may be minor disturbances in the overall structure, however no significant distortions or tidal features are observed, suggesting no major merging event is currently occurring.
