The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a concentrated luminosity, appearing as a bright, yellowish core. This suggests a likely concentration of older stellar populations in the galactic nucleus. The galaxy displays an elongated shape. There is little evidence of distinct spiral arms or strong dust lanes, lending credence to a classification of an early-type galaxy. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo or envelope. Slight asymmetry suggests minor gravitational disturbances. The galaxy appears relatively isolated.
