The galaxy appears to be part of a small group or interacting system. A primary galaxy, seen approximately face-on, exhibits a generally smooth, elliptical morphology. There is a concentration of light in the central region, suggesting a core or nucleus. The galaxy has an overall yellowish color profile. It is of average size and contains roughly 10^10 solar masses. The rate of star formation is slow. 

A secondary galaxy, located nearby, is viewed edge-on or at a high inclination angle. This galaxy displays a flattened disk-like structure, hinting at spiral morphology, although definitive spiral arms are not discernible in this image. This secondary galaxy has a bluer color profile than the primary galaxy. This galaxy has a medium size and appears to be undergoing some sort of disturbance.

A third, smaller and much dimmer object is visible. It is most likely another galaxy, but it could be a star cluster.

The system shows evidence of gravitational interaction, potentially evidenced by distortions in either galaxy's morphology. It does not appear to be in the late stages of merging, but in an early stage.
