The galaxy presents an elliptical morphology, appearing as a somewhat elongated spheroid. The light profile suggests a smooth distribution of stars, with a centrally concentrated bulge. There's a color gradient visible, trending towards redder hues in the central region and slightly bluer colors towards the periphery. The overall color suggests a mature stellar population. No prominent spiral arms or dust lanes are discernible. The structure appears relatively undisturbed, without significant signs of tidal interactions or major mergers. There is evidence of ongoing star formation at a very low rate. The object appears to be a relatively massive system.
