The galaxy presents as a centrally concentrated object with a smooth overall appearance, exhibiting a high degree of symmetry. It possesses a flattened, elliptical shape, tending toward a more rounded, rather than elongated, form. The galaxy's light profile suggests a bulge-dominated morphology, with a relatively bright central region that gradually fades into the outer regions. There's a subtle color gradient observed, with a slightly redder hue in the central bulge and a bluer tint in the surrounding disk. This suggests a difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars present within the disk. Faint wisps or irregularities are visible, possibly indicating minor disturbances.
