The object presents as a relatively smooth, centrally concentrated galaxy with a generally elliptical morphology. The light distribution indicates a dominant spheroidal component, possibly a large bulge. There's a slight elongation to the overall shape, moving it away from a perfectly circular appearance, but it isn't strongly barred or obviously disk-like. Color gradients appear subtle, with a slightly redder hue towards the center and a somewhat bluer (though still muted) color in the outer regions. This could indicate older stellar populations dominating the core, with some ongoing or recent star formation occurring in the surrounding areas. There is no strong evidence of significant tidal interactions or major disturbances in the galaxy's morphology.
