This galaxy presents as a disk galaxy, although its exact classification is somewhat ambiguous due to its irregular structure and disturbed appearance. The galaxy exhibits a flattened, elongated morphology, but lacks well-defined spiral arms. The central bulge is not prominent, and the light distribution suggests a rather low central mass concentration.

Distinctly blue regions are scattered throughout the galaxy, indicating areas of active star formation. These regions likely contain young, hot, massive stars emitting strongly in the blue part of the spectrum. There are hints of faint dust lanes interspersed within the disk, obscuring some of the background light.

There's also evidence of a possible minor disturbance in the disk, perhaps due to a minor merger or tidal interaction with another galaxy. Overall, this galaxy seems to be experiencing an ongoing, albeit not exceptionally vigorous, period of star formation within a somewhat disrupted structure.
