The galaxy presents as a roughly elliptical object. The central region is a bright, diffuse glow. There are also faint star forming regions around it. Based on the color, the galaxy is likely old and not actively forming stars. There is no clear disk structure or spiral arm morphology, but the presence of some bluer regions suggests some on-going star formation. There is no major ongoing merger activity, but there are some signs of minor disturbance. The light distribution is primarily concentrated in the core, with a gradual decrease in brightness towards the edges. The galaxy appears generally smooth and well-defined.
