The galaxy exhibits a somewhat elongated morphology. Its color profile appears predominantly bluish-white, with a brighter central region suggestive of a concentrated stellar population. A faint, extended halo surrounds the core. The structure is not perfectly smooth; some irregularities or disturbances appear present in the outer regions, indicating possible gravitational interactions or recent merger activity. The overall visual impression suggests a galaxy that may be in an intermediate stage of evolution, possibly transitioning from a more active star-forming phase to a more quiescent state.
