The galaxy presents an elongated morphology with a notable asymmetry. A brighter, more concentrated central region is visible, suggesting a galactic bulge, though its exact form is difficult to discern. The galaxy appears to exhibit a relatively smooth profile, with a gradual decrease in surface brightness from the center outwards. The overall color is bluish, indicative of recent or ongoing star formation, although the presence of dust lanes or spiral arms cannot be definitively confirmed at this resolution. There is a subtle indication of disturbance in the galaxy's structure; however, more data is needed to determine if this is a genuine interaction or an internal feature of the galaxy. The galaxy is relatively compact, with the majority of its light concentrated within a small area.
