The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. There is a clear central bulge that emits a yellowish light, potentially indicating a high concentration of older, cooler stars. Fainter, more diffuse regions extend outwards from the central bulge. These outer regions exhibit a subtle change in color, appearing slightly bluer, hinting at the presence of younger stellar populations. The galaxy appears to be generally rounded in shape, with minimal signs of significant disturbance or tidal features indicative of recent major merger events. Overall, the galaxy gives the impression of a mature system that is undergoing, at most, only minor star formation.
