The galaxy presents as a relatively smooth, elliptical form with a high degree of central concentration. Its color profile suggests an older stellar population, particularly in the central bulge, which exhibits a yellowish hue. The outer regions of the galaxy show hints of bluer colors, possibly indicating some ongoing, albeit subdued, star formation. There is no strong evidence of spiral arms or significant dust lanes. The galaxy's morphology appears largely undisturbed, lacking signs of major mergers or tidal interactions. Its overall structure suggests a galaxy that is relatively evolved, possibly in the process of transitioning towards a red and dead state, with a declining star formation rate. The apparent elongation indicates a moderate degree of ellipticity.
