The galaxy presents as a centrally concentrated system with a diffuse, extended halo. The core exhibits a yellowish hue, potentially indicating an older stellar population and a lower rate of current star formation within this region. The outer regions of the galaxy appear less structured and more irregular, with hints of bluer colors, suggesting the presence of younger stars and ongoing star formation. The galaxy's shape is approximately round, but not perfectly spherical. There's a slight elongation and subtle asymmetrical features in the outer regions, possibly hinting at minor gravitational interactions or disturbances. Overall, the galaxy appears relatively smooth, but close examination reveals some faint, diffuse features. There are no obvious signs of a major merger.
