The galaxy presents as a somewhat elongated, possibly disc-shaped structure. Its central region appears smoother and more concentrated, with a color gradient transitioning from a yellowish hue at its core to a bluer tint in its outer regions. This color gradient might indicate variations in stellar population, with older, redder stars concentrated towards the center and younger, bluer stars populating the periphery, potentially indicating ongoing, albeit moderate, star formation. The smoothness suggests a more evolved system where spiral arms, if present, are not well-defined or are tightly wound. There are slight signs of asymmetry or minor disturbances in the overall structure, possibly hinting at past interactions or internal dynamical processes.
