The galaxy presents as a spiral type, with distinct, albeit somewhat flocculent, spiral arm structures. There is evidence of ongoing star formation within these arms, noticeable by the presence of regions exhibiting bluer colors. The galaxy's disk is oriented at a moderate inclination, not quite face-on, but also not fully edge-on, allowing a partial view of its spiral structure. A prominent bulge is present, contributing significantly to the overall light profile of the galaxy, but not dominating the overall visual structure. There is a possibility of interaction or a minor merger event, indicated by some distortion in the outer disk or arm structures. The galaxy appears to have no strong bar feature.
