The galaxy presents as a single, moderately bright object, exhibiting an elliptical morphology. The light distribution appears relatively smooth, with a concentrated central region, decreasing in intensity towards the outer edges. The galaxy's shape deviates slightly from perfectly circular, showing a hint of elongation. No distinct spiral arms or bar structures are discernible. There is no clear evidence of a major merger event, although there may be minor perturbations in its morphology. Overall, it appears to be a relatively undisturbed system.
