The galaxy presents an ellipsoidal morphology, appearing relatively smooth with no prominent spiral arm structures immediately discernible. It exhibits a yellowish-orange hue, suggesting a population of older stars and a lower rate of ongoing star formation. The shape is mostly round, with a minor elongation present, tending towards a cigar shape. A possible interaction or merger is suggested by the galaxy's irregular outline, with one dominant and one minor nucleus, indicating two separate galactic structures. A likely merger event is undergoing, or completed, with the two structures now one. The system exhibits a high luminosity. The image is likely showing a system where the mass is high but the star formation rate is low, consistent with a later-stage galaxy evolution.
