The galaxy presents as a merging system, characterized by two distinct components. The primary component appears as a relatively smooth, bright spheroid with a yellowish hue. The secondary component, located nearby, exhibits a bluer color, suggesting ongoing star formation activity. There is strong visual evidence of tidal disturbance between the two objects, indicating gravitational interaction. Given the overall morphology and the presence of two interacting components, the galaxy likely exhibits a moderate stellar mass. Despite being visually disturbed, the galaxy is neither perfectly spherical nor highly elongated, showing an intermediate shape.
