The galaxy presents as a spiral type, viewed at an angle that is somewhat face-on. There is evidence of a central bulge which appears relatively compact and moderately prominent. The spiral arms are not tightly wound; they are more open and defined. The overall color suggests an intermediate population of stars. The disk shows some degree of patchiness, possibly indicating regions of ongoing star formation. There is no obvious evidence of a major merger event. Some asymmetry is present, potentially indicating a minor interaction or internal disturbance. The galaxy's shape deviates from a perfectly smooth elliptical profile, suggesting the presence of substructure within the disk. There is a possibility that the galaxy contains a bar structure. 
