The galaxy appears to be a relatively luminous object at a considerable distance, exhibiting a somewhat smooth morphology. A dominant central bulge, characterized by a yellowish-red hue, suggests a population of older stars. There may be low star formation as indicated by some blue light, though older stars are dominating the light output. The overall shape is largely circular, deviating only slightly from perfect roundness, and shows a smooth, elliptical shape. There is some possible tidal disturbance observed, potentially indicative of a minor interaction or recent merger. The system exhibits a complex structure, possibly involving subtle distortions or asymmetries.
