The observed galaxy presents a relatively compact morphology. There is no clear disc structure, nor any obvious spiral arms. The galaxy appears somewhat amorphous in shape. The light distribution seems brightest in the center and diffuses outward. The color profile appears uneven with some areas more green. Some features suggest a possible merger event, perhaps a minor disturbance that resulted in the clumpy light distribution. The galaxy shows a subtle indication of a tidal tail or arm.
