The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light is concentrated in a bright central bulge or core, with a color profile that leans towards the redder end of the spectrum, potentially indicating an older stellar population with relatively suppressed star formation activity. The outer regions of the galaxy appear more diffuse, lacking any distinct spiral arm structures or prominent dust lanes. There may be some minor disturbances due to interaction or merging. It displays a moderate degree of roundness, without a distinctly elongated shape.
