The galaxy presents a largely smooth and rounded morphology. It exhibits a concentrated central bulge that dominates the overall light profile. There's a hint of a flattened disk component surrounding the bulge, but the disk appears relatively featureless. The color index suggests a population of older stars. Faint, disturbed light around the galaxy hints at a possibility of a past merger. Overall, the galaxy appears as a relatively evolved system, likely an elliptical or lenticular galaxy, with minimal ongoing star formation.
