The galaxy presents as a merging or interacting system composed of two distinct components. The first component exhibits a smooth, relatively featureless morphology, with a concentrated, yellowish core indicative of an older stellar population. The second component appears bluer and more diffuse, potentially indicative of ongoing star formation activity. There's evidence of gravitational disturbance between the two components, possibly in the early stages of a merger. The overall shape of the system is irregular, deviating significantly from a typical spiral or elliptical morphology. The system's faintness suggests that this galaxy is relatively distant.
