The galaxy exhibits a complex morphology, appearing as a central, somewhat irregular structure with a significantly brighter, elongated component extending from one side. The overall color suggests active star formation regions, particularly in the more diffuse areas.

The galaxy appears to be undergoing some form of interaction or disturbance, as the central region shows signs of asymmetry and possibly tidal features. The elongated component has a smoother, more uniform distribution of light, possibly indicating an older stellar population or a tidal tail created through past interactions. Light from the galaxy's central region indicates older stars.

The galaxy has an estimated redshift of 0.063396, indicating a relatively nearby object in the grand scheme of cosmological distances. Further analysis and higher resolution imaging would be necessary to fully understand the nature of the interactions and star formation history of this system.
