The galaxy presents a generally smooth appearance, with a subtle, elongated shape. The central region exhibits a brighter, more concentrated luminosity, suggesting a significant concentration of stars toward the galactic nucleus. The light smoothly decreases in intensity away from the center. The galaxy appears relatively undisturbed, with little evidence of ongoing major mergers or tidal interactions. It exhibits hints of disk structure, but primarily has an elliptical or lenticular morphology. Overall, the galaxy demonstrates a largely quiescent state, with a moderate rate of star formation. The estimated size of the galaxy is approximately 6 kpc.
