The galaxy presents a predominantly smooth morphology, with a concentrated central bulge and a more diffuse surrounding halo or disk. The overall shape is somewhat elliptical, deviating slightly from a perfect circle. Color gradients suggest a centrally concentrated population of older, redder stars, which transitions to a bluer population in the outer regions of the galaxy. There is a subtle indication of a disk-like structure, though no distinct spiral arms are visible. No significant disturbances or signs of recent merger activity are immediately apparent in the image. The galaxy exhibits a relatively even light distribution across its structure, with a smooth transition from the bright central bulge to the fainter outer regions.
