The galaxy presents a largely smooth morphology, with a generally elliptical shape. The central region exhibits a strong concentration of light, appearing a yellowish-orange hue, suggesting a population of older stars. The outer regions display a gradual decrease in surface brightness, fading into the background. There is no prominent spiral arm structure visible, nor are there any distinct dust lanes. There are no obvious signs of tidal disturbances, such as streams or tails, which would indicate recent merger activity, although subtle irregularities in the outer halo cannot be ruled out. Based on the observed colors, the galaxy likely possesses a relatively low star formation rate overall.
