The galaxy presents as a somewhat elliptical morphology, appearing as a spheroid with a moderate degree of central concentration. Its color profile is dominated by warmer hues, suggesting an older stellar population. There is a subtle hint of a disk-like structure or feature, but is subtle. Perturbations exist, which suggests possible minor disturbance with a possible companion, or recent merger. The smooth appearance may indicate it is closer to an elliptical galaxy than a spiral, and the warmer colors may indicate an older and less active stellar population. 
