The galaxy presents a centrally concentrated light profile, suggesting a significant bulge component. The overall shape appears elliptical, trending towards roundness rather than a highly elongated form. Some subtle, diffuse features are visible in the surrounding disk, hinting at some form of structure beyond a purely smooth profile. There is no evidence of spiral arm structure or any significant active galactic nucleus. Faint disturbances visible in the galaxy's halo suggest minor interaction events or internal dynamical processes are likely occuring. The color profile shows some blue-ish tinges, which indicates some active star formation is likely happening within the galaxy. 
