The galaxy presents a largely smooth morphology, with a concentrated central bulge that dominates the overall structure. There is some evidence of a disk-like structure extending outwards, but it is not clearly defined and appears relatively faint. The galaxy appears to be mostly round in shape. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. A distinct, redder region is visible, possibly indicating an area of dust obscuration or a population of older, redder stars. There may be a minor interaction or disturbance affecting the overall shape.
