This galaxy exhibits a somewhat disturbed morphology, potentially indicative of an ongoing or recent merger event. A central, brighter region appears present, surrounded by more diffuse, less defined structure. The distribution of light suggests a relatively irregular shape, lacking the clear spiral arms or elliptical form of more settled galaxies. Distinct bluer regions are observed suggesting areas of more active star formation. There are a few faint tidal features or streams of stars extending outwards, providing further support for an interaction or merger. The galaxy displays a relatively low overall surface brightness with notable asymmetry.
