The galaxy presents a largely smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge that transitions into a fainter, more diffuse halo. The color profile indicates an aging stellar population, with a dominant reddish-orange hue in the core and diminishing towards the outer regions. There is little evidence of spiral arm structure or significant dust lanes. Slight perturbations in the galaxy's overall shape suggest potential minor gravitational interactions or past merger events, though the dominant structure remains relatively undisturbed. The galaxy appears to have a low rate of star formation, judging by the lack of bright blue regions indicative of young, hot stars. 
