The galaxy presents as a predominantly smooth and rounded structure, suggesting an elliptical morphology. The central region exhibits a concentrated luminosity, indicating a substantial stellar density or possibly an active galactic nucleus. There is a subtle elongation observed, hinting at a deviation from perfect circularity and a possible transition to a lenticular (S0) type galaxy. Faint, diffuse extensions are visible surrounding the core, potentially representing a stellar halo. There is no clear indication of prominent spiral arms or significant dust lanes, which further supports the classification as an early-type galaxy. The galaxy is of considerable size, appearing relatively large for its redshift and suggestive of a substantial stellar mass. The overall color is reddish, consistent with an older stellar population and a relatively low rate of ongoing star formation.