The galaxy presents as a luminous, elongated structure, suggestive of an elliptical or lenticular morphology viewed at an oblique angle. A smooth, centrally concentrated bulge dominates the light profile, exhibiting a yellowish hue. The outer regions gradually fade into the background, with a subtle color gradient indicating slightly bluer outskirts. The absence of well-defined spiral arms or significant dust lanes supports the classification as an early-type galaxy. There is no visible sign of active galactic nuclei activity and little evidence of recent or ongoing star formation within the galaxy's disk. Overall, this galaxy appears to be an evolved stellar system with a substantial mass and a quiescent star-formation history. It is notable that one side of this galaxy has what appears to be a slight disturbance. This could be a satellite dwarf galaxy slowly merging, or tidal interactions with another galaxy.
