The galaxy presents a spiral morphology, exhibiting discernible spiral arms. These arms appear somewhat loosely wound, displaying active star formation regions. The star formation activity is suggested by the presence of bluish hues distributed throughout the arms, which could indicate younger, hotter stars. A moderate bulge is noticeable at the galaxy's center, displaying a yellowish hue indicative of an older stellar population. The galaxy does not appear to be undergoing any major mergers, though there are possible signs of minor disturbances within the disk. No prominent bar structure is evident. Overall, this galaxy appears to be a spiral galaxy with a moderate bulge and ongoing star formation within its spiral arms.
