The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated light profile. There is a gradual decrease in surface brightness from the core outward, lacking any prominent spiral arms or distinct features, though there is a slight disk-like structure. The central region appears bright and yellowish, suggesting an older stellar population. The galaxy exhibits a slight red-shift, indicating it is not within our immediate galactic neighborhood. The light distribution indicates a fairly evolved system, likely with a substantial mass. There are suggestions of some minor gravitational disturbance.
