The galaxy appears as a moderately bright, centrally concentrated object. The light distribution suggests a roughly elliptical morphology. There is a smooth appearance, with no obvious spiral arms or a prominent disk-like structure. The central region shows a higher concentration of light, potentially indicating the presence of a bulge. Color gradients are subtle, but there appears to be a slight reddening towards the center. No significant dust lanes or signs of ongoing mergers are visibly apparent, suggesting a relatively undisturbed system. The object is relatively compact in angular size.
