The galaxy presents a centrally concentrated luminosity profile, suggestive of an early-type morphology. The primary body of the galaxy appears smooth and relatively featureless, lacking prominent spiral arms or well-defined dust lanes. A notable, smaller secondary concentration of light is visible, possibly indicating an ongoing or recent minor merger event, or an area of localized star formation. The overall shape tends towards elliptical, but with slight deviations from perfect roundness. The galaxy's color is predominantly yellow-orange, hinting at an older stellar population with reduced ongoing star formation. Subtle disturbances in the outer regions may suggest gravitational interactions. The image suggests a galaxy undergoing a transformation process, possibly moving from a more actively star-forming state to a passively evolving state.
