The galaxy presents as a dual system, likely interacting. The primary component exhibits a smooth, elliptical morphology, with a concentrated, bright core. The color is predominantly yellowish-white, indicative of an older stellar population. The secondary component displays a disk-like morphology with a notable reddish hue, suggesting the presence of dust and possibly ongoing star formation. There appears to be a faint tidal bridge or connection between the two galaxies, indicating gravitational interaction. The size of the primary component is moderately larger than the secondary disk galaxy. Overall, the system displays signs of mild disturbance, though not a fully developed major merger.
