The galaxy presents an elliptical morphology, appearing smooth and relatively featureless across its visible extent. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting a population of older stars. The outer regions display a fainter, bluer color, hinting at the presence of some younger stellar populations and perhaps a lower level of ongoing star formation within the galaxy's disk. The galaxy appears somewhat elongated, deviating slightly from a perfectly circular shape, likely due to its intrinsic structure and angle of observation. There is no obvious presence of spiral arms or significant dust lanes; its overall structure indicates a more evolved galaxy with a substantial stellar mass.
