The galaxy presents a smooth, centrally concentrated morphology, appearing largely featureless without prominent spiral arms or a distinct disk structure. It exhibits an elliptical-like shape with moderate roundness, showing only subtle deviations from a perfect circle. The galaxy's color profile is somewhat homogenous across its body, possibly indicating an older stellar population. There is no sign of a recent or major merger, but the possibility of minor disturbances may need further investigation. The galaxy's overall appearance suggests a system that has largely settled into a stable configuration, lacking strong signatures of ongoing star formation.
