The galaxy presents an overall elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. It exhibits a concentrated central bulge that displays a yellowish hue, suggesting a population of older, redder stars dominating this region. The light gradually diffuses outwards from the core, transitioning into a fainter, bluer halo. This suggests the presence of a younger stellar population and possibly some ongoing star formation in the outer regions, although at a low rate. There is a slight elongation in the galaxy's shape, suggesting it is not perfectly spherical. There is no evidence of any major ongoing merger events or significant tidal disturbances. The galaxy appears relatively undisturbed.
