The galaxy presents as a somewhat symmetrical object, roughly elliptical in shape, although there's a slight irregularity to the distribution of light. The central region appears brighter and more concentrated, suggesting the presence of a galactic bulge. Moving outwards from the center, the intensity of light decreases gradually, transitioning into a fainter and more diffuse halo.

There's a subtle color gradient visible within the galaxy. The central bulge exhibits a yellowish hue, possibly indicating a population of older, redder stars. Surrounding the central region, there is a hint of bluer light, perhaps suggesting the presence of younger stellar populations or regions of ongoing star formation, though it is not prominent. No distinct spiral arm structure or well-defined features are discernible. 

The overall appearance is indicative of a mature galaxy. There is no strong evidence of recent major mergers or tidal disturbances affecting the system. The structure appears relatively settled.
