The galaxy appears to be a spiral galaxy, exhibiting distinct spiral arm structures. These arms are somewhat tightly wound, emanating from a central bulge. The bulge is moderately sized. There is potential evidence of a bar structure bisecting the central region, although it is not prominently defined. The disk is viewed at a slight angle, but not perfectly edge-on. The galaxy shows no prominent signs of major mergers, but minor disturbances in the spiral arm structure are discernible. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The spiral arms display bluer colors indicative of ongoing star formation. The overall morphology does not seem to be of a perfectly elliptical or smooth kind, however, there is some smoothness exhibited in the central region.
