The galaxy presents as a relatively smooth, rounded object. There is no apparent disk structure or spiral arms visible at this resolution. The central region exhibits a higher luminosity, suggesting a concentration of stars or an active galactic nucleus. The galaxy shows a slight color gradient, with the core appearing more reddish-yellow, transitioning to a bluer hue in the outer regions. There are no obvious signs of recent major merger activity or significant tidal disturbances, though subtle irregularities in the outer isophotes could hint at minor interactions or internal asymmetries.
