The galaxy presents as a spiral type, exhibiting a distinct disk structure. The spiral arms are prominent, with evidence suggesting multiple arms emanating from the central bulge. These arms are tightly wound.

The central bulge appears moderately sized in relation to the disk. The overall color profile indicates active star formation, with blue hues concentrated in the spiral arms and a yellower tone in the central bulge, potentially indicative of an older stellar population in that region. There is no obvious presence of a bar structure, but the central region appears to be somewhat elongated. 

The galaxy appears relatively undisturbed, lacking any major signs of ongoing merger activity or significant tidal distortions in its overall morphology. There is a suggestion of minor disturbance, but the galaxy appears relatively normal.
