The galaxy presents as a spiral type, with a bright, concentrated central bulge that appears yellowish.  Spiral arms are clearly visible, exhibiting a tightly wound structure. The arms display a flocculent morphology, with patchy regions of blue coloration suggestive of active star formation. The disk appears relatively face-on. There is no obvious sign of a strong bar structure bisecting the central bulge, though a faint elongated structure may be present. Evidence of ongoing interactions or major disturbances is not immediately apparent, although there are minor irregularities and asymmetries in the arm structure. The overall color gradient indicates that the bulge is populated by an older stellar population, while the arms contain younger, bluer stars. The galaxy exhibits a moderate inclination. There appears to be a small central bulge within a larger bulge area.
