The galaxy presents as a singular, relatively compact object. It exhibits an overall elliptical morphology, though not perfectly spherical; there is some elongation. The light distribution appears quite smooth, suggesting a lack of significant spiral arm structure or prominent dust lanes. Color gradients are subtle. There appears to be a slight concentration of light towards the center, implying a central bulge or core. No obvious signs of ongoing major merging events are apparent, but a hint of minor asymmetry or tidal features cannot be completely ruled out given the image resolution. The overall color suggests a population of older stars, with a smaller contribution from younger, bluer stars. The galaxy is likely an early-type galaxy.
