The galaxy presents as a somewhat elliptical structure, dominated by a smooth, centrally concentrated bulge. The color profile suggests a relatively old stellar population, indicated by the yellowish-red hue of the central region. There is a faint, elongated, bluish extension that appears to originate from the main body of the galaxy. This could indicate a tidal tail or a plume of material ejected during a past interaction, or perhaps a region of younger stars. The overall morphology suggests a system that may have undergone some past gravitational disturbance, although it presently appears relatively undisturbed. The lack of distinct spiral arm structure suggests that it is likely an early-type galaxy, possibly an elliptical or lenticular type. The small size of the system may indicate that the star formation rate is low. 
