The galaxy presents as a smooth, elliptical morphology. It appears elongated, with an approximate axis ratio indicating a deviation from a perfectly circular shape. The light profile is centrally concentrated with a gradual falloff in intensity towards the edges, characteristic of an early-type galaxy. There is no discernible spiral arm structure or evidence of a prominent disk. The galaxy exhibits a relatively uniform color distribution, with a slightly bluer central region. There are no obvious signs of active galactic nuclei activity or significant dust lanes. The overall appearance suggests a galaxy that has undergone substantial evolutionary processing, potentially having exhausted much of its gas reservoir and exhibiting a low star formation rate. There is a slight possibility of a minor disturbance in the galaxy's structure, but most likely there is no ongoing or recent major merger event occurring within the system.
