The galaxy presents as a spiral type, viewed at a moderate inclination relative to our line of sight. Evident spiral arms are visible within the disk, exhibiting a somewhat flocculent structure. The disk component appears dominant, with the presence of a moderate-sized central bulge. The bulge is noticeably redder than the disk. Evidence of a bar structure is present within the central region of the galaxy, although the definition is somewhat weak. The overall morphology suggests a system that has not experienced recent major merging activity, although there might be slight morphological disturbances present. The galaxy has a relatively small estimated radius. The integrated color indicates a galaxy with significant star formation activity.
