The galaxy presents a generally smooth morphology with a slight disk-like or featured component. Its overall shape is somewhere between round and in between round and cigar shaped, but closer to the round classification, showing some degree of elongation. There may be signs of some disturbance such as a potential minor disturbance or merger event. The color suggests a moderate amount of ongoing star formation. The galaxy exhibits a noticeable central bulge, with a fainter, more diffuse halo extending outwards. The light distribution suggests a significant population of older stars in the core, surrounded by a region with relatively younger stellar populations.
