The galaxy presents an irregular morphology, showing evidence of interaction and possibly a merger event. A primary, more luminous component is observed, exhibiting a yellowish hue, indicative of an older stellar population. Below this component, there is a secondary, less luminous region that is significantly bluer in color, which could indicate a region of active star formation. There are tidal disturbances that appear faint and hard to make out, and are very asymmetrical. The overall shape deviates considerably from a regular elliptical or spiral form, further supporting a scenario where gravitational interactions and ongoing mergers are influencing the galaxy's structure.
