The galaxy presents a spiral morphology, observed at a slight inclination. The disk component exhibits spiral arms, though their structure appears somewhat flocculent. A prominent central bulge is present, showing a high degree of symmetry and smooth luminosity profile. The galactic disk appears relatively thin and is the dominant morphological feature. The color gradient suggests active star formation regions within the spiral arms, with subtle indications of dust lanes. There is no obvious evidence of a strong bar structure. Overall, the galaxy appears to be a late-type spiral with a moderate-sized bulge.
