The galaxy presents a largely smooth, elliptical morphology. It appears to be relatively compact, displaying a concentrated central bulge which seems to smoothly fade into the outer regions of the galaxy. The color gradient shows a generally yellow-orange hue in the core, possibly indicating an older stellar population. The outer regions of the galaxy suggest a subtle transition to a slightly bluer hue, hinting at the presence of some younger stars, though not indicative of significant star formation. There is little evidence of spiral arms or disk-like structures; instead, the galaxy exhibits a near-uniform, slightly elongated shape. No obvious signs of major ongoing mergers are apparent. There might be a very slight hint of minor tidal disruption, but this is difficult to definitively determine from the image alone. Overall, this galaxy appears to be a massive, evolved system with a moderate redshift, suggestive of ongoing, but low, star formation.
