This galaxy appears to be an interacting system. The primary component exhibits a generally rounded morphology. The light distribution is concentrated towards the center, appearing almost spherical, and decreasing in intensity outwards. A secondary component can be distinguished, situated nearby. This is an apparent disturbance of the primary body, showing an asymmetrical light distribution suggesting either a tidal interaction or a smaller galaxy in the process of merging. The colour index suggests the presence of both young, blue star-forming regions and older, redder stellar populations within the primary galaxy. The secondary component shows similar characteristics. Overall, the galaxy system presents a disturbed morphology, indicative of a dynamic and potentially ongoing merging process.
