The galaxy presents as a single, dominant, relatively smooth and centralized object. The light profile appears largely elliptical and exhibits a radial color gradient, transitioning from a bluer hue towards the periphery to a more yellow and red color at the core. This suggests a population of older stars concentrated in the central region. There is evidence of some slight distortion, possibly indicative of a minor interaction with a smaller companion galaxy. An elongated, diffuse object is visible close by. It's elongated morphology and bluer color suggests a possible tidal tail or a separate galaxy undergoing tidal disruption. The primary galaxy shows some clumpy regions which might indicate sites of modest star formation. Overall, the galaxy appears to be a relatively massive system, with a low rate of star formation and a significant fraction of its stellar mass concentrated in a spheroidal component.
