The galaxy appears to be a spiral galaxy, observed at an angle slightly off from face-on. The central bulge seems moderate in size and possesses a yellowish-white color, suggesting an older stellar population. The spiral arms are readily apparent, displaying a somewhat tightly wound structure. They are populated with regions of active star formation, marked by a blueish hue indicative of younger, hotter stars. These regions are not uniformly distributed across the arms, but rather appear as distinct clumps. There may be two dominant arms. The dust lanes within the spiral arms are not prominently visible, which implies a more settled structure. There's no obvious evidence of a prominent bar structure. There doesn't seem to be any major signs of any merger events. The color indices suggest relatively strong star formation rates.
