The galaxy presents as an elliptical or lenticular type, exhibiting a predominantly smooth morphology. There is a slight elongation in its shape, but it is mostly classified as in between round and cigar shaped. Its color gradient suggests a population of older stars, with a concentration of redder hues dominating the central bulge. The galaxy shows no signs of strong recent or ongoing star formation. There is no obvious indication of any significant merger events or major disturbances affecting its structure, although there is some visual indication of a potential minor disturbance.
