The galaxy exhibits a primarily smooth morphology with a relatively small angular size. The light distribution appears centrally concentrated, transitioning smoothly outwards. The core of the galaxy displays a bright, almost point-like source. The galaxy appears to be generally redder towards the center and bluer towards the outer regions. There is evidence of faint, extended emission surrounding the central region, creating a halo-like appearance. The galaxy does not show any obvious signs of strong spiral arm structures or a distinct disk. There is very little, if any evidence of a recent or ongoing major merger. There is a faint, almost ring like shape. The galaxy is not completely featureless, hinting at possible internal substructures or irregularities, though these are subtle.
