The galaxy presents as a singular, moderately bright object with an approximate angular diameter of 2 arcseconds. The light distribution suggests a relatively smooth morphology, lacking distinct spiral arms or a pronounced central bulge. There's an appearance of two central components, each being similarly bright, which could indicate an ongoing or recent merger event. The overall colour is yellowish, which would suggest an older stellar population and reduced active star formation. A faint, disturbed structure is visible around the central part of the object, which might be part of an ongoing merging process. 
