The galaxy presents a largely smooth morphology, appearing elliptical in shape. There is a notable central bulge, brighter and slightly redder in color than the surrounding disk. The disk exhibits a bluer hue, indicative of younger stellar populations or ongoing star formation. The galaxy does not appear to show strong evidence of spiral arms or significant dust lanes. There may be a very slight disturbance in the light profile indicating a potential past minor merger. Overall, the galaxy has a relatively regular and undisturbed appearance.
