This galaxy presents as a centrally concentrated, relatively smooth object. The core region exhibits a bright, almost unresolved appearance, suggesting a high stellar density. Moving outward from the center, the galaxy displays a gradual decrease in surface brightness. 

The overall shape appears somewhat elliptical, with the major and minor axes being fairly similar in length, giving it a close-to-round morphology. There is a subtle hint of a disk-like structure, but it is not prominently defined.

The color profile suggests a population of older stars, primarily concentrated in the core. Fainter, bluer regions exist within the outer halo, possibly indicating ongoing or recent star formation in those areas.

There's a slight asymmetry to the galaxy’s morphology. It could potentially be interacting with another galaxy, but the lack of strong tidal tails or other obvious signs suggests a minor disturbance. The edges of the galaxy are diffuse and indistinct, fading gradually into the background sky.
