The galaxy presents as a lenticular or possibly a spiral galaxy seen at an oblique angle. It exhibits a generally smooth, elliptical light profile, with a noticeable elongation. There is a subtle suggestion of a disk structure. No significant dust lanes or prominent spiral arm structures are visually apparent. The galaxy's color appears slightly blue-ish or white, suggesting the presence of a young stellar population, but this is not strongly pronounced. The general morphology suggests a galaxy that is either an early-type spiral or a transition object between elliptical and spiral types. The relative smoothness suggests a galaxy that has undergone significant processing and lacks ongoing major star formation, which could be confirmed by an estimated star formation rate of approximately 10^-0.2 solar masses per year. The estimated stellar mass is approximately 10^10 solar masses. There might be some minor asymmetry within the galaxy's light distribution, which could indicate a past or ongoing minor interaction or disturbance, but this is not immediately obvious.
