The galaxy presents as an elliptical morphology, with a smooth and concentrated central bulge, and a faint disk. It exhibits a moderate axial ratio, appearing somewhat elongated. The core is characterized by a yellowish-white hue, suggesting an older stellar population. Progressing outwards from the core, the disk reveals a gradual shift towards redder tones and eventually diminishing intensity, which suggests that the star formation rate is relatively low compared to its mass. There is no strong evidence of spiral arm structure or prominent dust lanes. No major merger events are visible, only minor disturbances. Overall, it seems to be a fairly undisturbed system.
