The galaxy presents as a single, largely homogenous object. Its overall morphology appears smooth and elliptical, with a high degree of circularity. A bright, concentrated core is visible, surrounded by a more diffuse halo.

Color gradients are subtle but present. The central region exhibits a yellowish-white hue, possibly indicative of an older stellar population. Moving outward, a slight shift towards bluer tones is observed, which might suggest younger stars or ongoing star formation at a low rate within the galactic outskirts.

There is a notable absence of distinct spiral arms, bars, or prominent dust lanes. No signs of major disturbances, tidal tails, or interactions with other galaxies are readily apparent.

The galaxy's apparent size indicates a considerable physical scale. The galaxy seems to be well-isolated in its environment.