The galaxy presents a generally smooth appearance, lacking strong spiral arm structures or a prominent central bar. There is evidence of a possible disk or faint features within the galaxy. The shape approximates a rounded form, though not perfectly circular, with a slight elongation. The light distribution appears concentrated towards the center, indicative of a bulge. Colors suggest a population mix; there are hints of bluer regions, possibly indicating younger star formation, alongside the yellower/redder hues associated with older stellar populations and dust. It is not currently undergoing a major merger, though signs of minor disturbances cannot be ruled out entirely, based on the slight asymmetry present in the outer regions of the galaxy.
