The galaxy presents a predominantly smooth morphology, with minimal discernible features such as spiral arms or a prominent disk structure. Its shape is generally elliptical, appearing more rounded than elongated, with a slight tendency towards an intermediate form between perfectly circular and highly elongated. There are no obvious signs of recent or ongoing major mergers. However, there may be slight visual asymmetry, possibly indicating a minor disturbance or interaction, though the galaxy’s overall structure remains largely undisturbed. The galaxy emits light across the visible spectrum, with a slightly enhanced emission in the blue-green region, which may indicate the presence of some recent star formation.
