The galaxy presents as a diffuse and somewhat irregular object. The light profile appears centrally concentrated, but without a distinct nucleus. The overall color is relatively blue, suggestive of ongoing star formation. There is a hint of morphological disturbance, as evidenced by faint, elongated features possibly indicating tidal interactions or ongoing mergers. There is also a hint of disk-like structure, however the irregularities are more prominent. Overall, the galaxy does not appear to be a classic spiral or elliptical type. It has a size of approximately 16 kpc. The estimated stellar mass suggests a typical galaxy on the main sequence of star forming galaxies at its redshift.
