The galaxy presents as a roughly elliptical structure, with a bright, concentrated core region exhibiting a primarily white luminosity. This central area is surrounded by a somewhat diffuse halo, transitioning into a turquoise hue and extending outwards. Irregularities in the outer structure suggest potential tidal disturbances or interactions. There is a subtle asymmetry in the distribution of the outer halo, possibly indicative of recent or ongoing mergers or minor disturbances affecting the overall morphology. Overall, the galaxy appears to be relatively compact.
