The galaxy presents a somewhat irregular, but generally disk-like morphology. The object exhibits a relatively bright central region that appears to be a modest bulge. Spiral arm structures appear present but are somewhat diffuse and patchy. The overall color of the galaxy leans toward bluer wavelengths, possibly indicating a relatively younger stellar population and ongoing star formation. It shows a slightly elongated shape, with a visible tilt relative to our line of sight. There appear to be some disturbances to the shape possibly due to a minor merging event. The light emitted from this galaxy is consistent with other galaxies within a comparable redshift range.
