The galaxy presents as a spheroid with a high degree of central concentration, exhibiting a smooth, elliptical morphology. Color gradients are subtle, transitioning from a yellowish core to slightly redder hues in the outer regions. Evidence suggests a relatively old stellar population, implying a cessation of significant recent star formation activity. There is a potential, minor gravitational disturbance from a nearby object. The galaxy lacks a prominent disk or spiral structure and has a high degree of roundness. There are no obvious signs of active galactic nuclei activity or significant dust lanes. 
