The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth, elliptical morphology. The core region displays a high surface brightness, appearing bright yellow, which likely indicates an older stellar population. A gradual decrease in surface brightness is observed moving outwards from the core. There is a very faint hint of an outer halo. The overall shape is somewhat elongated. There are no obvious signs of spiral arms, bars, or significant dust lanes. No major merging events or tidal disturbances are apparent, although a slight asymmetry cannot be entirely ruled out. The galaxy appears fairly isolated.