The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. The core is bright and slightly blue-shifted, potentially indicating the presence of a population of younger stars or ongoing star formation, although at a low rate. The outer regions of the galaxy show a gradual decrease in surface brightness, transitioning to a redder hue, suggestive of an older stellar population. Overall, the galaxy presents a generally undisturbed morphology, lacking any significant tidal features or evidence of recent major merger events. It appears fairly round, with no apparent asymmetry.
