The galaxy presents as a diffuse, extended object with an apparent red shift. A dominant central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. A fainter, somewhat elongated disk-like structure extends outward from the central bulge, exhibiting a bluer tint hinting at younger stars and ongoing star formation, though at a relatively low rate. This outer region contains some disturbances or possible merging components as indicated by asymmetry and irregular shapes, and the disk appears relatively smooth. The roundness is hard to tell from this angle. There is a possibility of minor disturbances or a merger event, as the morphology does not appear entirely relaxed or symmetrical. The overall impression is of a galaxy that has a significant spheroid component and a relatively calm ongoing star formation.
