The galaxy appears as a relatively small, elongated object. It exhibits a smooth, centrally concentrated morphology, with a gradual decrease in surface brightness from the core outwards. The galaxy's overall color is slightly redder, suggesting a population of older stars. There is little evidence of active star formation regions or distinct spiral arm structures within the observable light. The galaxy does not appear to be significantly disturbed or undergoing a major merger event, however there may be a slight disturbance.
