The galaxy presents as a somewhat disturbed system. The morphology appears irregular, possibly indicative of an ongoing or recent interaction. There is a defined central bulge that is moderately bright, suggesting a substantial population of older stars. Extending outwards from this bulge are fainter features that could be attributed to the galaxy's disk, but they appear warped or disrupted. Blueish hues can be seen which may indicate areas of active star formation, particularly in the outer regions of the disk-like structure. Patches of what could be dust and gas are visible within the structure.
