The observed galaxy appears to be a spiral galaxy exhibiting a moderate inclination relative to our line of sight. A prominent central bulge is observed. The spiral arms appear to be well-defined, extending outwards from the central bulge. I note the presence of an apparent two well-defined spiral arms. The arms also appear to exhibit a medium degree of winding. There is also the possibility of minor disturbances present, but it is difficult to confirm with certainty. The galaxy does not appear to be a merger. Overall the features observed indicates disk-like morphology with ongoing star formation.
