The galaxy presents as a relatively smooth, elliptical morphology. The light distribution is centrally concentrated, exhibiting a gradual falloff in intensity outwards from the core. The overall color appears yellowish-orange. There is a slight asymmetry in the outer isophotes, suggesting the possibility of a minor tidal interaction or past merger event. There is no obvious active star formation within the galaxy based on the color, but the integrated color implies a largely older stellar population with a low specific star formation rate. The galaxy displays a notable apparent size, with the possibility of being an early-type galaxy. There are no clear indications of spiral arms, a prominent disk structure, or a strong central bar. The appearance is consistent with a galaxy that has undergone significant morphological transformation, possibly transitioning toward a more quiescent state.
