The galaxy presents as a relatively smooth, elliptical structure. Its core appears luminous and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population dominating the central region. Moving outward from the core, the color transitions to a more diffuse, greenish-yellow glow. This indicates the presence of some younger stars, though their contribution seems less significant than the older population in the core. 

There is little evidence of spiral arms or significant dust lanes. A small distortion or asymmetry might be present on one side of the galaxy, although this is subtle. The overall structure indicates a system that has likely undergone significant merging or internal relaxation, leading to its current spheroidal shape. The star formation appears relatively low. The galaxy is located at an intermediate distance, evidenced by its redshift.
