The galaxy presents a somewhat disturbed morphology, potentially indicating an ongoing or recent interaction. The light distribution is not uniform, with an elongation and a hint of tidal features, possibly tails or bridges of stellar material extending from the main body. There appears to be a dual core-like structure. One is red-shifted and one is slightly blue-shifted. The galaxy exhibits a range of colors, including a redder, presumably older stellar population, alongside regions that appear bluer, suggesting the presence of younger stars or active star formation. The overall structure is fuzzy, lacking sharp, well-defined edges. The relatively smooth light distribution in some regions could indicate a significant spheroidal component, while the bluer regions suggest the presence of spiral arm fragments or irregular star-forming regions. The redshift suggests this galaxy is not a local object, implying a considerable distance.
