The galaxy appears to be an elliptical galaxy, exhibiting a largely featureless, smooth morphology. The light distribution suggests a high degree of central concentration. It presents a round shape, showing no evidence of disk-like structure or spiral arms. The color gradient indicates a population of older stars, as is expected in elliptical galaxies, with a redder hue towards the central bulge. There is no evidence of any major merging events or tidal disturbances. The galaxy appears to be relatively isolated and undisturbed.
