The galaxy presents as a moderately luminous object with an apparent diffuse morphology. It exhibits a dominant smooth structure with some indication of a disturbed morphology, such as minor tidal features, potentially indicating an ongoing or recent interaction or merger event. The light distribution suggests a centrally concentrated bulge component with an extended, but ill-defined disk. The overall color appears to be on the redder side, suggesting an older stellar population with relatively suppressed star formation activity. The shape appears to be generally rounded, but not perfectly spherical. There is a suggestion of multiple nuclei, or possibly regions of higher density within the galaxy itself, but there is evidence of features that may point to a system that is either merging or recently has done so.
