The galaxy presents a primarily smooth morphology, with a slight deviation from a perfectly circular shape. It appears somewhat in between circular and elliptical. The galaxy exhibits a dominant central bulge characterized by a bright, concentrated region of light. This central region displays a yellowish-orange hue, potentially indicating an older stellar population. Subtle disturbances are present, possibly suggesting interactions with smaller galaxies or previous merger events. The overall color suggests a relatively low rate of star formation. Based on the observed features, this galaxy is likely a massive, relatively evolved system.
