The galaxy presents an overall elliptical morphology. A smooth, centrally concentrated bulge dominates the galaxy's structure, exhibiting a yellowish-white hue. This suggests an older stellar population in the core. The outer regions display a fainter, bluer tinge, hinting at the presence of some younger, hotter stars, possibly within a weak, diffuse disk component. There is only the slightest possible hint of spiral structure. The galaxy is not perfectly spherical; instead, it appears slightly elongated. There appears to be little to no sign of recent or ongoing major mergers or significant tidal disturbances based on the image's morphology, although it is not completely smooth.
