The galaxy presents as a relatively compact object with a smooth, diffuse appearance. There is a bright, concentrated central region that suggests the presence of a galactic nucleus. The overall shape is somewhat elliptical, though not perfectly spherical, with a moderate degree of roundness. There is no apparent spiral structure or distinct disk component visible. The galaxy exhibits a subtle color gradient, transitioning from a bluer hue in the central region to slightly redder tones in the outer fringes, which may indicate differences in stellar populations or dust content across the galaxy. There is no obvious evidence of a major ongoing merger or significant tidal disturbances. The overall structure hints at an evolved system that is potentially a transitioning spiral or an elliptical type galaxy.
