The galaxy appears to be an elliptical galaxy, characterized by a smooth, largely featureless morphology. It exhibits a centrally concentrated luminosity profile, fading gradually towards the outer edges. There is a slight bluish tint to the galaxy, but the core region is more white, perhaps implying an older stellar population with ongoing, but diminished, star formation, with small concentrations of younger stars. The shape is mostly round with minimal elongation or distortion, although there is a hint of disturbance. Evidence suggests that there has been no major merging event. Given the absence of prominent spiral arms or a distinct disk structure, and the smooth, spheroidal appearance, this system aligns with a classification towards the early-type end of the Hubble sequence.
