The galaxy exhibits a generally smooth morphology, appearing mostly featureless. The light distribution suggests a central concentration of older stars, indicated by the yellowish-white hue at the core. The overall shape is more rounded than elongated, though not perfectly spherical. There are indications of some ongoing or recent interaction, possibly a minor disturbance or early stage merger with a smaller object, represented by asymmetrical features or tidal arms. These features are very dim but potentially indicative of star formation. The galaxy appears moderately massive, with an inferred mass of approximately 10^11 solar masses. Its estimated star formation rate, though not exceptionally high, indicates active star formation.
