The galaxy presents a smooth, elliptical morphology, appearing relatively undisturbed. It exhibits a concentrated central bulge that dominates its overall structure. The galaxy's light profile gradually fades outwards from the core without any prominent spiral arms or other distinct features. The color appears slightly redder, suggesting an older stellar population. The roundness of the galaxy appears to be in between round and elliptical. There appears to be no indication of ongoing major merging activity, although there might be very minor disturbances.
