The galaxy presents a roughly elliptical morphology, appearing relatively compact within the observed field. The central region exhibits a bright, concentrated core, suggesting a high density of stars or an active galactic nucleus. 

Moving outward from the core, a subtle disk-like structure can be discerned, although it is not clearly defined. There appears to be slight color variation within the galaxy's structure. The central core displays a cyan hue.

The outer edges of the galaxy show faint disturbances or tidal features, hinting at possible gravitational interactions. The slight asymmetry in the outer regions further supports this observation.
