The galaxy presents an overall smooth morphology, appearing largely featureless. It exhibits an elliptical shape, leaning towards roundness. The light profile appears concentrated towards the center, with a gradual decrease in brightness towards the outer edges. There is a slight indication of some minor internal disturbance within the galactic structure, but no major signs of an ongoing merger event are immediately apparent. The galaxy presents a color gradient, transitioning from a bluer central region to redder hues at the periphery. The estimated size would make this a relatively average sized galaxy. The strong blue light indicates a relatively high rate of recent star formation. The overall mass of the galaxy is likely substantial.
