The galaxy presents as a system comprised of what appears to be a main galaxy and at least two distinct luminous components in close proximity. The main galaxy is elongated, potentially a disk galaxy seen at a significant inclination. Its light is reddish-orange, suggesting an older stellar population or significant dust obscuration. The two neighboring components, exhibiting similar coloration to the main galaxy, are less defined, appearing more diffuse in their light distribution. They are situated to either side of the main galaxy, possibly representing tidal features or smaller galaxies in the process of merging. The general morphology leans toward a system that may have undergone or is currently undergoing interaction or merging events. Star formation appears to be occurring at a modest rate. The overall smoothness indicates a relatively evolved system.
