The galaxy appears to be a merging system, exhibiting a disturbed morphology. The primary component is a relatively smooth, elliptical-like structure, appearing elongated along a particular axis. There is a clear color gradient across this structure. The core appears to be composed of old stars.

A secondary component is also visible, and it appears smaller and more compact. This component displays a reddish color, potentially indicating an older stellar population or significant dust obscuration. There is evidence of gravitational interaction between these two structures.

The overall system lacks well-defined spiral arms or a prominent disk structure. The light distribution suggests a relatively low rate of ongoing star formation, consistent with a system dominated by an aging stellar population. There's potential evidence of tidal features extending outward from the system, suggesting past or ongoing interactions, although image resolution limits definitive identification.
