The galaxy appears as a somewhat elongated structure with a diffuse, smooth morphology. There is a suggestion of a disk, but the dominant feature is a relatively featureless central bulge. The galaxy exhibits a color gradient, appearing bluer in the outer regions and becoming redder towards the core, indicative of potential variations in stellar populations or dust content. A faint, extended halo may be present, though its boundaries are poorly defined. There seems to be a minor tidal disturbance, or a faint merger occuring.
