The galaxy presents as an elliptical system, exhibiting a smooth, diffuse morphology without prominent spiral arms or a distinct central bulge. The light distribution is centrally concentrated, fading gradually towards the outer edges. The shape appears elongated, with a moderate degree of ellipticity. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue, with a lack of significant blue coloration that would signify recent star formation. There are no apparent signs of ongoing mergers or tidal disturbances.
