The galaxy presents a generally smooth appearance, with a slight elongation in its shape. The color distribution appears to be centrally concentrated, exhibiting a yellow-orange hue in the core, indicative of older stellar populations. Fainter blueish regions are observed asymmetrically along the periphery, potentially suggesting regions of more recent star formation. There appear to be no well-defined spiral arms or a prominent disk structure. The galaxy exhibits a moderate degree of disturbance.
