This galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy based on its morphology. The light distribution exhibits a noticeable radial gradient, with a bright, compact core that gradually fades into an extended halo. There is a slight elongation to the galaxy, with a moderate ellipticity. The galaxy has a dominant yellowish-orange color, possibly indicative of an older stellar population and a lack of significant ongoing star formation, but is still exhibiting some bluer tinges around the halo. There are no immediately obvious signs of strong tidal interactions or significant disturbances in its overall structure. The galaxy appears to be relatively isolated, with no obvious nearby companions within the immediate vicinity.
