The galaxy appears as a single, unresolved, elliptical-like entity. It is characterized by a smooth, centrally concentrated luminosity profile, showing a high degree of symmetry. The galaxy's color is a pale yellow-white, suggesting a moderate to high population of older stars with relatively little ongoing star formation. There are no visible spiral arms, dust lanes, or other prominent features typically associated with disk galaxies. The morphology implies it is likely an elliptical galaxy. A very small degree of interaction cannot be ruled out, but the galaxy's overall undisturbed appearance makes it unlikely that it is undergoing a major merger. The isophotes are generally round, indicating a low degree of ellipticity.
