The galaxy presents a generally smooth and rounded morphology. There is a concentrated central bulge that is bright and elliptical in shape. The color of the bulge is predominantly yellow, indicating an older stellar population with lower ongoing star formation. The galaxy exhibits no clear spiral arm structure or prominent dust lanes. The outer regions of the galaxy appear fainter and somewhat more diffuse, possibly indicating a gradual decrease in stellar density with increasing distance from the galactic center. There is no obvious signs of tidal disturbances, strong interactions with nearby objects, or a prominent disk component. The galaxy appears to be a relatively isolated elliptical galaxy with little ongoing star formation. 
