The galaxy presents as a diffuse object with a relatively small angular size. It exhibits a blue hue, suggesting a significant population of young, hot stars. The light distribution appears fairly uniform across the galaxy, with little to no evidence of a central bulge or distinct spiral arm structures. There are some subtle indications of disturbances within the galaxy's morphology, possibly hinting at ongoing or past merger events. These disturbances are visible as slight asymmetries in the light distribution. There may be faint tidal features present. The galaxy appears largely unstructured, suggesting it is likely undergoing a major interaction or in a post-merger state.
