The galaxy appears to be an interacting system composed of two distinct galactic structures. The primary galaxy exhibits an elliptical morphology, appearing relatively smooth in texture. The light is concentrated toward the center of the galaxy, suggesting the presence of an older stellar population. The color is skewed towards redder wavelengths, which also corroborates that interpretation.

Neighboring the elliptical galaxy is a fainter spiral galaxy with a bluish tinge to its arms. These arms display signs of distortion and fragmentation. The color suggests the presence of younger, hotter stars in the spiral arms. The nucleus of the spiral galaxy is also visible. 

The morphology of the two galaxies, and their proximity to each other, suggest gravitational interaction. The minor disturbances noted in the spiral structure may be tidal effects resulting from this interaction. The overall color profile suggests a mixed stellar population across the system.
