This galaxy appears to be an elliptical galaxy, characterized by its relatively smooth and concentrated light distribution. The central region exhibits a bright, yellowish glow, likely indicative of an older stellar population. The isophotes are generally elliptical in shape, with a noticeable deviation from perfect circularity. No distinct spiral arms or prominent dust lanes are visible, further supporting its classification as an elliptical. The galaxy appears largely undisturbed, lacking any significant tidal features or signs of ongoing mergers. The color profile suggests a red sequence galaxy, typical of passively evolving systems with low star formation activity.
