The galaxy appears as a relatively smooth, centralized structure. There's a subtle color gradient across the galaxy's body, hinting at varying stellar populations. The overall shape tends more towards circular, with minimal elongation. The overall color suggests a mix of stellar ages, with a possible dominance of older stars. There are indications of potential disturbances in its morphology, possibly suggestive of a minor interaction or past merger event. The galaxy exhibits an apparent magnitude that suggests it is moderately distant.