The galaxy presents as a spiral type, exhibiting a noticeable disk structure. The disk is not perfectly face-on, showing some tilt relative to the observer's line of sight. There appear to be spiral arms, though they are somewhat flocculent and not tightly wound. The color distribution suggests active star formation, as indicated by the bluer regions scattered throughout the disk. A central bulge is present but does not dominate the galaxy's overall appearance. There is some evidence of possible interaction or disturbance, with the disk showing some irregularities and asymmetries. It is possible this could be in the beginning stages of merging. The galaxy's light profile is consistent with a stellar mass in the range of approximately 10^9 solar masses, and it appears to be undergoing moderate levels of star formation. The current rate of star formation would classify it as being in the "green valley".
