The galaxy presents as a somewhat elliptical structure with a visible core. The luminosity appears greater in the center, gradually diminishing towards the outer regions. The color distribution indicates a potentially older stellar population concentrated centrally, exhibiting yellowish hues. The disk of the galaxy shows a bluer tint suggesting the possibility of more recent star formation in this region. The galaxy does not appear to show any signs of major mergers or significant tidal disturbances. The structure gives the impression of a relatively settled system. The angle of inclination suggests the galaxy is tilted toward our line of sight.
