The galaxy presents a largely smooth morphology with a centrally concentrated light profile. The overall shape appears close to round. There is a notable lack of distinct spiral arms or bar structures. The central region exhibits a bright, concentrated core, possibly indicative of a supermassive black hole or a dense stellar population. Moving outward from the center, the light gradually diffuses, with a transition towards a less luminous outer halo. No major disturbances or signs of recent mergers are immediately apparent, although there might be subtle asymmetries or irregularities within the outer regions that warrant further investigation. The color profile suggests a redder central bulge, becoming slightly bluer in the outskirts. The relatively smooth texture and color gradients hint towards an evolved stellar population.
