The galaxy presents an overall elongated, irregular morphology, indicative of a possible disk galaxy viewed at a significant inclination. The light distribution appears relatively smooth, with a moderate concentration towards the center. A subtle bluer color is observed in the central region, hinting at recent or ongoing star formation. The galaxy lacks prominent spiral arms. The outer regions are fainter and more diffuse, displaying a somewhat clumpy structure. There are slight indications of minor tidal disturbances around the galaxy, suggesting a possible past interaction. Overall, the object appears to be a low-mass, relatively faint galaxy, possibly experiencing a low level of star formation activity.
