The galaxy exhibits a clear spiral structure, with prominent spiral arms emanating from a central bulge. These arms appear somewhat fragmented and display a mix of morphologies, with varying degrees of tightness in their winding. Some arms are more tightly wound, while others are more loosely defined. The central bulge is moderately sized and emits a significant amount of light, suggesting a substantial stellar population.

There are indications of both ongoing and past star formation within the galaxy. Patches of bluer light are visible within the spiral arms, consistent with areas of active star formation. The overall color suggests a mixture of stellar populations, hinting at a galaxy with a complex evolutionary history.

The overall impression is that the galaxy is not undergoing a major merger, but there might be minor gravitational interactions or disturbances affecting its structure. These potential interactions could be influencing the distribution of gas and dust, and consequently the star formation activity within the spiral arms.
