The galaxy presents a generally smooth, rounded morphology. A concentration of light is observed toward the center, suggesting a prominent galactic nucleus. There is evidence of a slight elongation. Color gradients are subtle; however, the central region displays a yellow to orange hue which could imply an older stellar population. Fainter blue tinges are present in the outer regions which could indicate active or recent star formation. Overall, the galaxy lacks any obvious signs of spiral arms or significant irregular features. No clear evidence of an ongoing major merger is seen.
