The galaxy appears as a relatively compact object with a bright, concentrated core. There is a distinct color gradient, transitioning from a bright, cyan-colored center to a more yellow and red-tinged outer region. The overall structure seems largely spheroidal, with limited evidence of well-defined spiral arms or a clear disk-like morphology. The outer regions exhibit some irregularity, suggesting the presence of subtle disturbances or tidal features. The galaxy is likely an early-type galaxy or a spiral galaxy with a dominant bulge and tightly wound spiral arms. There is a possibility of a minor interaction, though the system appears predominantly undisturbed. The smooth appearance supports a classification toward the elliptical side of the Hubble sequence, or a face-on spiral galaxy. The bright central region could indicate an active galactic nucleus or a high rate of star formation in the nuclear region.
