The galaxy presents a largely smooth morphology, suggesting a relatively evolved system. Its overall shape appears to be somewhat elliptical, neither perfectly spherical nor highly elongated. A central bulge region is evident, exhibiting a yellowish hue, which might indicate an older stellar population. The outer regions of the galaxy are fainter and bluer in color, potentially indicative of ongoing or recent star formation, albeit at a seemingly low rate. There are no obvious signs of spiral arms or a prominent disk structure in this image. Furthermore, there is no clear evidence of major mergers or significant tidal disturbances impacting the system's overall structure. The galaxy appears to be a relatively isolated system, displaying a stable and undisturbed morphology.
