The galaxy presents a generally smooth and rounded morphology. There is a concentration of light in the galaxy's central region. Moving outwards, the light diffuses in all directions, giving the appearance of a somewhat elliptical shape with a slight elongation. The galaxy displays a color gradient, transitioning from a more yellowish-white core to a reddish halo. There is no visible evidence of spiral arm structure or significant disk features; the light distribution is relatively uniform without any major disturbances or ongoing mergers visible. The galaxy seems to be isolated, lacking prominent tidal tails or nearby interacting companions. The smooth appearance indicates an older stellar population, with relatively low star formation activity.
