The galaxy presents as a relatively smooth, elongated structure, possibly a lenticular or edge-on spiral galaxy, though the low resolution obscures fine details. Its color gradient suggests an aging stellar population, with a yellowish core that brightens considerably towards the center. There is a very faint suggestion of a disk, although it may simply be caused by the galaxy's ellipsoidal shape. There is no obvious dust lane nor visible star forming regions. The shape and color are consistent with a system that has experienced substantial evolution, with minimal on-going star formation. There appears to be no signs of interaction or recent merger activity, indicating a relatively isolated and undisturbed evolution.
