The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing somewhat elongated but predominantly round. The core region is the brightest part of the galaxy, with a yellowish-white hue, suggesting an older stellar population. There is a gradual decrease in brightness as we move outward from the center. Faint extensions of galactic material surround the bright center, indicating a halo of stars that extends beyond the primary body. There are no clearly defined spiral arms or a prominent disk structure, and the overall structure is relatively undisturbed with only subtle distortions, with no obvious signs of an ongoing major merger or significant tidal interactions. Based on these observations, this galaxy is likely a relatively massive, early-type galaxy with a low rate of star formation.
