The galaxy presents a primarily smooth morphology, with a slight elongation discernable from its overall shape. A dominant central bulge exhibits a concentrated, bright yellowish-white luminosity. The outer regions, or disk, exhibit a diffuse, less intense glow in reddish hues, gradually fading into the background. There is no evidence of a strong spiral structure, though a subtle disk component appears to be present, contributing to the overall shape. There are no prominent tidal features or obvious signs of a major merger event in progress, though some minor asymmetry cannot be ruled out. The galaxy is characterized by an estimated mass of 10^10 solar masses, it exhibits a relatively low rate of star formation.
