The object presents as a spiral galaxy, observed at a moderate inclination. There is evidence of a central bulge with a spheroidal morphology. The disk component exhibits defined spiral arms. The arm structures appear somewhat flocculent, with regions of star formation activity indicated by a blue color in these areas. Overall the galaxy shows a low surface brightness, with a slightly irregular morphology suggesting possible gravitational interactions or past minor merger events. There also appears to be a faint bar feature at the center, potentially indicating a higher density or star formation rate in that region.
