The galaxy presents as a relatively small, centrally concentrated object. A bright, approximately circular core dominates its appearance. It has a primarily smooth overall morphology. There is evidence of faint disturbances, though minor, appearing as subtle asymmetries or irregularities in the outer regions of the galaxy. The galaxy's color profile shifts from a bluer hue in the central region to redder tones in the extended outskirts, potentially indicating differing stellar populations or dust content across the galactic structure. Based on the observed features there may be a possibility of a recent or ongoing minor merger event.
