The galaxy presents a predominantly smooth morphology. It exhibits an elliptical shape, leaning towards a more flattened, disk-like structure, but with no clear spiral arms. The light distribution is fairly even across the galaxy, with a slight concentration towards the center. There is a hint of some minor disturbances, with a slight asymmetry in the light distribution, but no significant signs of a major merger or tidal disruption. Based on the color, it is comprised of an older population of stars. Given the lack of dust and gas, we can conclude that this galaxy has a low star formation rate. Based on the information, we can estimate this galaxy is fairly massive.
