The galaxy presents as a concentrated central region with a moderate angular size. There is a subtle disk-like structure present. The central region is the most prominent and brightest, showing a condensed core. There is evidence of some disturbance in the galaxy, possibly due to tidal interactions. The overall morphology suggests a galaxy undergoing some interaction or disruption with the presence of disk and a relatively smooth overall appearance. The color distribution suggests differential star formation rates across the galaxy, with bluer colors potentially indicating younger stellar populations.
