The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless profile. The core is concentrated, with luminosity decreasing outwards. The major to minor axis ratio suggests a generally rounded appearance, showing only a slight ellipticity. Color gradients indicate a redder central bulge which could mean there are older stars located in the center, and the presence of bluer, younger stars in the outer regions. There is no obvious evidence of spiral arms, bars, tidal tails, or significant dust lanes. The general morphology of the galaxy is undisturbed, suggesting a lack of recent major merger events or significant interactions.
