The galaxy presents as a generally smooth, elliptical structure with a centrally concentrated light profile. It exhibits a gradual decrease in luminosity outward from the core. The core appears nearly spherical, with a yellowish-white hue, suggesting an older stellar population dominating the central region. Moving outward, the galaxy displays a bluer color gradient, hinting at ongoing or recent star formation in the outer regions. There are no distinct spiral arm features or a prominent disk visible. Some minor asymmetry may be present but is indistinct. The overall morphology appears undisturbed, with no obvious signs of major mergers or tidal interactions.
