The galaxy presents as an elliptical morphology with a high degree of central concentration. The light distribution appears smooth and relatively featureless, showing no distinct spiral arms or bar structure. The color is generally yellowish-orange, with the central bulge exhibiting a brighter, more intense emission. There is a subtle color gradient, with the outer regions appearing slightly bluer compared to the core, indicative of some ongoing, though relatively limited, star formation. The shape is largely spheroidal, with only a minimal deviation from perfect roundness. There are no readily apparent signs of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated, with no immediately neighboring galaxies that would suggest a recent interaction, though some minor disturbances cannot be excluded. Given the color and smooth appearance, it is likely to be a relatively massive galaxy comprised of older stellar populations.
