The galaxy presents as a relatively smooth, centrally concentrated light distribution. The morphology appears to be primarily elliptical or spheroidal. There is a noticeable color gradient from a yellowish-white core to a more muted, greenish-yellow outer region. The absence of defined spiral arms or significant dust lanes supports a classification as an early-type galaxy. The galaxy does not show obvious signs of tidal disruption or merging events, although subtle asymmetries cannot be entirely ruled out given the image resolution. The overall shape suggests a relaxed system with minimal ongoing star formation.
