The galaxy appears to be relatively small and compact. The central region exhibits high surface brightness, appearing quite bright and unresolved in this image. There's an extended, less luminous halo surrounding the core. The morphology appears somewhat disturbed. Faint extensions or tidal tails are visible suggesting possible minor merger activity. The color profile indicates a generally blue hue, most prominent in the central regions, suggesting recent or ongoing star formation. There also appears to be some indication of dust lanes or patchy obscuration near the center of the galaxy. The smoothness of the galaxy is low, implying the existence of stellar populations or structures. The apparent disturbance also indicates that the galaxy may not be in a state of equilibrium.
