The galaxy presents as a spiral type, exhibiting a prominent, moderately sized bulge at its core. The bulge displays a yellowish hue, indicative of an older stellar population. Two distinct spiral arms emanate from the central bulge, appearing tightly wound near the core and gradually loosening as they extend outwards. The spiral arms exhibit a bluer color, suggestive of ongoing star formation activity. Patches of intense star formation are visible along the spiral arms. The disk of the galaxy presents a slight inclination relative to our line of sight, allowing us to observe both the bulge and spiral arm structure. There is evidence of a bar-like structure in the center of the galaxy. There also appears to be some distortion, which may indicate a recent interaction with another object, possibly a minor merger.
