The galaxy presents a roughly elliptical morphology with a high degree of central concentration. It exhibits a smooth light distribution, lacking prominent spiral arms or bar structures. The color profile suggests a prominent bulge component that is redder in color, surrounded by a fainter, bluer disk or halo. There's a suggestion of potential disturbances in the outer regions of the galaxy, hinting at possible past or ongoing interactions. The overall color and smooth morphology indicate an evolved stellar population, though the presence of bluer light in the outer regions suggests ongoing or recent star formation.
