The galaxy appears as a centrally concentrated object, likely an elliptical galaxy, based on its smooth, featureless morphology. There is a strong central bulge that graduates into the outer edges of the galaxy, which appear less bright. The overall color appears to be on the redder side. The galaxy appears to be isolated; there is no evidence of tidal tails or distortions in the image. This may indicate that the galaxy has not recently undergone a major merger event or experienced strong gravitational interactions with other galaxies. The light distribution suggests that the galaxy is mostly comprised of older stars. Based on the light, the galaxy likely has a suppressed rate of star formation. The shape of the galaxy is neither distinctly round nor elongated. The structure seems undisturbed, with no major disruptions visible.
