The galaxy exhibits a morphology suggestive of a spiral type, though with some irregularities. A discernible disk component is present, but the orientation is neither perfectly face-on nor edge-on. Faint spiral arm structures are suspected within the disk, appearing somewhat diffuse rather than tightly wound. The central bulge appears moderate in size, contributing significantly to the overall luminosity of the galaxy. There is an indication of a possible weak bar structure across the bulge, although this is not definitively confirmed. There may be some ongoing interaction or merging event affecting the galaxy's structure, as indicated by an irregular shape and possible tidal features. There are some areas of blue which may indicate ongoing star formation.
