The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the light profile, exhibiting a yellowish hue. There is little evidence of spiral arm structures or prominent dust lanes. The outer regions of the galaxy appear more diffuse, fading gradually into the background sky. The galaxy exhibits a slightly elongated, though mostly circular, shape. There are no obvious signs of tidal disturbances, major mergers, or ongoing star formation in the arms. The color distribution suggests an aging stellar population.
