The galaxy presents an elliptical morphology with a smooth, centrally concentrated light distribution. A pronounced bulge component is evident, exhibiting a yellowish hue indicative of an older stellar population. There appears to be a slight elongation along one axis, but the overall shape remains largely spheroidal. The outer regions show a gradual decrease in surface brightness, fading into the background. There is no apparent spiral arm structure or significant dust lane obscuration, which supports the classification as an elliptical galaxy with little current star formation. No significant signs of ongoing mergers or tidal disturbances can be detected.
