The galaxy presents an overall elliptical morphology with a smooth, concentrated light profile at its core. The central region exhibits a bright, cyan-colored nucleus, potentially indicative of an active galactic nucleus (AGN) or intense star formation. Surrounding the nucleus, a gradual transition to a warmer, yellow-orange hue is observed, which might represent an older stellar population and/or dust obscuration.

A subtle disk-like structure may be present but it is difficult to fully resolve due to the galaxy's orientation. Evidence of possible tidal features or minor disturbances is visible in the form of faint extensions or irregularities in the outer regions, suggesting a past interaction or merger event. Faint bluish regions appear asymmetrically positioned around the central body, possibly indicating the presence of younger stellar populations or regions of ongoing star formation. The overall color suggests a mix of stellar populations and potentially ongoing or recent star formation activity, alongside indications of possible past merger activity.
