The galaxy appears to be a relatively smooth, elliptical-type galaxy with a concentrated central bulge. The galaxy exhibits a generally round morphology, with a slight deviation from perfect circularity. There's no strong evidence of significant spiral arm structure or a distinct disk component. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards. There might be some minor distortions or disturbances in the outer regions. The galaxy presents a moderate level of star formation activity. The overall color is somewhat redder, suggesting a population of older stars. The galaxy is a large, massive system.
