The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. Its shape is somewhere between round and elliptical, displaying a slight elongation. There are no obvious spiral arms or disk-like structures visible. The light profile suggests a relatively smooth and gradual decline in intensity from the core to the outer regions. A hint of disturbance within the galaxy is present, though major mergers do not appear to be occuring. The galaxy is relatively luminous, and it likely demonstrates moderate star formation activity based on its color profile.
