The galaxy presents an overall elliptical morphology, suggesting a classification as an elliptical galaxy. The light distribution appears relatively smooth, with minimal evidence of distinct spiral arms or a prominent central bulge. There is a very minor disk-like structure that appears to be rotating. There are no major features indicating a recent or ongoing major merger event, but there appears to be a very minor disturbance that is causing the slight rotation of the disk-like structure. The central region is somewhat brighter than the outer regions, consistent with a greater concentration of stars toward the galactic nucleus. Color gradients are subtle, with the central region exhibiting slightly bluer tones, possibly indicative of younger stellar populations compared to the more reddish, older stars in the outer halo. The object's size appears relatively compact, and its overall structure suggests a well-evolved system, potentially with limited ongoing star formation. There appears to be a minor merging event taking place.
