The galaxy presents an asymmetrical morphology with an apparent disk-like structure. There are hints of spiral arms, but they are poorly defined. The galactic center appears to be somewhat brighter and more concentrated than the outer regions, and has a redder hue. The outer regions exhibit a bluer hue. The galaxy appears relatively isolated with no strong signs of tidal disruption or ongoing major merger activity. There is an asymmetry or disturbance in the galactic disk, which suggests possible minor interactions or internal processes. The overall color suggests a mix of stellar populations, with a more aged population centrally and younger stars in the disk. The smooth fraction indicates that it has some attributes of an elliptical galaxy, but the featured disk component is noticeable. Overall, the classification points to an intermediate type between a spiral and an elliptical galaxy.
