The galaxy presents a largely smooth morphology, with a dominant central bulge exhibiting a yellowish hue, suggesting a population of older stars. The overall shape is somewhere between round and cigar-shaped, with a slight elongation noticeable. Faint disk-like structure is visible, but not dominant. There is no major disturbances or presence of merging, but there are some minor disturbances present. There is little evidence of ongoing or recent star formation.
