The galaxy appears to be an interacting system, possibly undergoing a merger. One component presents a smoother, more amorphous morphology, exhibiting a yellow-orange hue suggestive of an older stellar population. The other component appears bluer, indicating ongoing or recent star formation. The bluer component exhibits some signs of tidal disruption, further supporting the interaction hypothesis. The overall structure is disturbed, lacking a clear spiral or elliptical shape. The system displays a moderate luminosity. The system has an approximate size around 5 kpc. There might be an artifact present within the galaxy.
