The galaxy presents as a centrally concentrated, relatively smooth object. Its overall shape is somewhat elongated, approaching a cigar-like morphology, but it appears mostly in between a round and cigar shape. The central region is a bright, concentrated bulge, appearing nearly white, indicative of an older stellar population. The outer regions display a bluer hue, possibly indicating the presence of younger stars or active star formation, though the rates of star formation seem relatively low. There are subtle hints of a disk-like structure, but it is not clearly defined. There is a slight possibility of minor gravitational interaction or disturbance in its overall morphology, although no distinct tidal tails or merger remnants are clearly visible. The galaxy shows a higher presence of older stars with lower ongoing star formation.
