The galaxy presents as a relatively compact structure with a centrally concentrated bulge. The primary color of the galaxy appears to be a blend of blue and white, indicative of ongoing star formation, although the light may be from an older stellar population as well. A faint disk structure is visible, with an irregular shape that does not display grand spiral arms. The overall morphology suggests a galaxy that may have experienced some form of recent disturbance or minor merger event, evidenced by the somewhat disrupted disk and features in the overall light distribution. The light emitted suggests moderate mass and low star formation.
