The galaxy presents as an elongated, cigar-shaped structure. There is a central bulge that exhibits a smoother, more diffuse light distribution, suggesting an older stellar population. Extending from this central region is a fainter, disk-like component with hints of spiral arm structure, although the resolution makes it difficult to discern clear spiral patterns. There are areas of intense blue, and also orange-red, suggesting active star formation. Overall, the galaxy displays a moderate level of disturbance, potentially indicating past or ongoing interactions. There appears to be a small tidal feature or possible merger event as the structure is not perfectly smooth and uniform. The galaxy's overall luminosity is moderate, typical of spiral galaxies at its approximate redshift.
