The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The shape is generally in between a perfectly round and a elongated shape, trending towards round, with only slight deviations from circular symmetry. The galaxy appears relatively undisturbed, showing no significant signs of ongoing mergers, major disturbances, or tidal features that would indicate recent interactions. The color profile suggests a dominant population of older stars, potentially indicating low star forming properties and a lower abundance of dust.
