The galaxy presents as a moderately luminous, lenticular-like structure, exhibiting a central bulge that is noticeably brighter and appears yellower than the surrounding disk. There's an indication of a flattened disk component, though the resolution does not allow for a definitive assessment of spiral arm structures. The morphology appears to be transitioning between an elliptical and spiral type, based on a somewhat smooth profile with hints of a disk. There are signs of some minor gravitational disturbance within the disk, as there are slight irregular light formations along the edges of the galaxy. Color gradients suggest the presence of older stellar populations concentrated within the bulge, transitioning to younger, bluer stars in the outer disk regions. The galaxy is not undergoing a major merging event, but is likely undergoing slow accretion of material.
