The galaxy presents a largely smooth morphology, with a high degree of central concentration. It appears elliptical in shape, exhibiting a round form. The galaxy shows a color gradient, transitioning from a redder core to bluer outer regions. There is no apparent spiral arm structure or distinct dust lanes. No major signs of tidal disturbances or ongoing mergers are observed, although there is a slight asymmetry that indicates a potential minor disturbance. Based on the color profile, star formation appears to be concentrated mostly within the galaxy's outer regions. The galaxy is relatively compact, occupying a small area in the frame.
