The galaxy appears to be a relatively smooth, elliptical galaxy with a slight elongation. Its core is a bright, concentrated region exhibiting a bluish-white hue, which may indicate a population of younger, hotter stars or active galactic nucleus activity. The surrounding halo fades gradually into the background sky. There is some evidence of faint, diffuse structure or tidal features extending from the main body of the galaxy. Given its overall morphology and observed color profile, this galaxy likely represents a moderately massive system with ongoing, but potentially low, levels of star formation. It exhibits no strong signs of major mergers or significant disruption.
