The galaxy presents an overall elliptical morphology, appearing elongated with a high degree of axial ratio. The central region exhibits a concentrated luminosity, indicating a likely bulge component. Proceeding outwards, the light gradually diffuses from the center, transitioning into a faint, extended envelope. There is a slight reddish hue in the central region of the galaxy, which may suggest a population of older stars in the bulge. The outer regions show bluer colors in the upper and lower regions of the galaxy, with a greater concentration on the bottom, potentially indicating regions of active star formation. The overall structure appears relatively undisturbed, with no obvious signs of ongoing major mergers or significant tidal interactions. This is likely a somewhat quiescent galaxy.
