This galaxy exhibits a primarily smooth morphology with a slightly elongated, though generally rounded, shape. The central region displays a strong concentration of light, appearing with a yellowish hue, suggestive of an older stellar population dominating the core. The outer regions fade gradually, showing a bluer tint, potentially indicating younger stars or ongoing star formation at the galactic periphery, though the effect is minimal. There are hints of minor disturbances in the outer disk, possibly tidal effects or minor interactions, but no major merger events are evident. Overall, the galaxy appears to be a relatively undisturbed system, potentially transitioning from a more actively star-forming state to a more quiescent one.
