The galaxy presents a morphology consistent with a spiral type, exhibiting a noticeable disk structure. Two prominent spiral arms emanate from a moderately sized central bulge, winding loosely around the galactic core. The arms are well-defined and display a degree of patchiness indicative of ongoing star formation. The bulge appears relatively bright and concentrated, potentially indicative of an older stellar population. There appears to be a faint bar like structure in the center of the galaxy. There are no signs of major disturbance or ongoing merger activity, however, there are signs of minor disturbances in one arm which suggests a potential gravitational interaction with a smaller mass object. There is a general smooth appearance, with no strong presence of dust lanes.
