The galaxy presents a somewhat irregular morphology, appearing neither perfectly elliptical nor a well-defined spiral. Its light distribution is relatively smooth, but with a noticeable feature, possibly a distortion or arm-like structure. The general shape appears somewhere between round and elongated. There may be some minor disturbance or merger activity occurring, based on the irregularities. The core of the galaxy appears compact and relatively bright. Color gradients suggest a redder central region, likely indicative of an older stellar population, with bluer outskirts suggestive of ongoing or recent star formation. The overall color indices indicate a dominant population of evolved stars, although younger stars are likely present.
