The galaxy presents a somewhat elliptical morphology. There appears to be a slight asymmetry to its overall shape, possibly indicating a past or ongoing interaction or merger event. The light distribution across the galaxy is not uniform; there is a bright, concentrated central region that could indicate a bulge. Moving outward from the center, the light appears to become more diffuse. The galaxy's color suggests a population of older stars with some ongoing star formation, or a significant dust component reddening the light. There might be a faint disk structure. Overall, the galaxy exhibits features consistent with a relatively massive system.
