The galaxy presents as a single, primarily smooth object with a slightly elliptical morphology. The color profile suggests the presence of older stellar populations, indicated by the reddish hue. There is a hint of bluer regions which may suggest a minor amount of ongoing star formation. There are no immediately apparent signs of spiral arms or a prominent disk structure. There may be a very faint, slight disturbance to the shape but it is difficult to definitively determine if the galaxy is undergoing a merger or experiencing tidal interactions.
