The galaxy presents as a flattened, elliptical structure with a smooth, diffuse appearance. It exhibits a central concentration of light that gradually fades towards the outer edges, suggesting a prominent bulge. The galaxy appears elongated, with an axis ratio indicating it is not perfectly spherical. There are subtle color gradients observed within the galaxy, with a slightly bluer hue in the outer regions compared to the central, redder core. This might indicate the presence of younger stellar populations in the outer disk. There is also an area in the center that appears bright pink which could be an area of star formation. Overall, the galaxy's morphology hints at a lack of significant ongoing mergers or major disturbances.
