The galaxy presents an overall elliptical morphology, appearing largely smooth and featureless in this image. The light distribution indicates a centrally concentrated profile, with a gradual decline in brightness moving outwards from the core. There is a subtle colour gradient, shifting from a yellowish-orange hue at the core to a fainter, slightly redder tint in the outer regions. This suggests an older stellar population dominating the central bulge, with possibly ongoing, low-level star formation occurring further out. There is no evidence of spiral arms or a well-defined disk, nor any distinct signs of recent major merger events. Based on its smooth appearance and colour profile, this galaxy is likely a relatively evolved system with a significant population of older stars. Faint asymmetrical features surrounding the galaxy could potentially point towards a minor disturbance or interaction with a companion galaxy, however, the resolution of this image is insufficient to be certain.
