The galaxy presents a somewhat diffuse, irregular morphology. It exhibits a mostly smooth appearance with little to no indication of prominent spiral arms or a well-defined galactic disk. It appears generally rounded, though not perfectly circular, trending towards a slightly elongated shape. The light distribution is centrally concentrated, but there are hints of subtle disturbances in the outer regions. The galaxy's color suggests a stellar population of intermediate age, with no overwhelmingly dominant blue or red hues. The galaxy may be undergoing minor gravitational interactions or internal disturbances, leading to its irregularity.
