The galaxy presents a predominantly smooth morphology, appearing largely spheroidal in shape. It exhibits a concentrated central bulge, radiating a yellow-white hue, indicative of an older stellar population. The outer regions display a gradual decrease in luminosity, suggesting a diffuse halo. Faint blueish tinges are observed, potentially indicating regions of lower, though still present, star formation. There is no discernable spiral structure or significant dust lane obscuration. Minor disturbances or signs of tidal interactions appear absent. The galaxy appears relatively isolated and well-defined, with a dominant spheroidal shape.
