The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light profile suggests a fairly elliptical shape, approaching circularity. There is a distinct core of yellowish-white light at the center, which likely indicates an older stellar population. The outer regions of the galaxy exhibit a gradual decrease in surface brightness. Some faint blue features are visible in the outer regions, which may indicate regions of ongoing star formation. There are no apparent spiral arms or a prominent disk-like structure visible. Based on the morphology, it can be classified as an early-type galaxy. Weak tidal features are present which is possible evidence of past or ongoing minor mergers.
