The galaxy presents as a relatively smooth, elliptical object with a high degree of central concentration. Its overall shape is elongated, exhibiting a cigar-like morphology. There is a bright, prominent core region that gradually fades into the outer regions of the galaxy. Hints of a disk-like structure might be present, but these are not strongly defined. There is no obvious evidence of recent or ongoing major merger activity, though there is a possibility of minor disturbances given the asymmetry in the faint outer halo. The galaxy's color profile transitions from a bluish white in the core to slightly redder hues in the outer regions, which may suggest regions of ongoing star formation.
