The galaxy presents a largely smooth morphology. It appears as an elliptical or lenticular system, exhibiting a centrally concentrated bulge region. The color gradient within the galaxy suggests some level of stellar population variation. The central region displays a reddish hue, potentially indicative of an older stellar population or dust obscuration. The outer regions are bluer, potentially representing a younger, star-forming population, although this could also be influenced by lower levels of dust extinction in the outer regions. The overall shape is somewhat elongated, with a slight deviation from perfect circularity. There might be a minor tidal disturbance or interaction occurring, though the signs are subtle. The galaxy's structure appears relatively undisturbed, without any major merging events.
