The galaxy exhibits a primarily smooth morphology, appearing as a concentrated central bulge, which dominates the overall structure. There is a slight elongation, but it is generally round. The light distribution appears relatively uniform with no prominent features like spiral arms or bars immediately evident in the image.

Color gradients suggest a redder center indicative of an older stellar population, transitioning towards slightly bluer hues in the outer regions. This might imply ongoing, though limited, star formation at the outskirts. There are no signs of recent major merger events. Weak tidal features may be present but they don't clearly suggest a merger is occurring. 
