The galaxy presents as a somewhat elliptical structure, with an elongated shape and a smooth, featureless appearance. A bright, concentrated core region is visible, suggesting a high stellar density and potentially the presence of a supermassive black hole. The color of the core is predominantly white, indicating a population of older, hotter stars.

Moving outward from the core, the galaxy exhibits a gradual decrease in surface brightness. The surrounding regions appear bluer in color compared to the core, suggesting the presence of younger stars. No distinct spiral arms or prominent dust lanes are apparent, which support the notion of a smooth overall morphology.

There is a very slight distortion in the galaxy's shape, suggesting the possibility of a past or ongoing interaction with another galaxy, though the galaxy seems primarily undisturbed. Overall, the galaxy is consistent with an early-type galaxy, likely an elliptical, with no major disturbances to the galaxy itself.
