The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the light profile. The outer regions appear less defined, with a gradual decrease in surface brightness, suggesting a diffuse halo component. There is a hint of a flattened, disk-like structure, however, this is not well defined. Based on the overall color profile, there seems to be a moderate amount of recent star formation activity within the galaxy, as indicated by the blueish hue. There is no evidence of significant tidal distortions or major merging events. Overall, the object appears to be a relatively undisturbed, evolving galaxy.
