The galaxy presents as a spiral type, exhibiting a prominent, elongated central bulge region exhibiting a yellow hue. Distinct spiral arms emanate from the central bulge, showing a relatively tightly wound structure. The arms themselves display a clumpy morphology, likely indicative of star-forming regions within the spiral arms. There appears to be a strong bar-like structure extending through the central region of the galaxy, aligning roughly with the major axis of the overall elongated shape. The disk of the galaxy shows signs of subtle disturbances, suggesting the possibility of minor gravitational interactions with another galaxy. The galaxy shows moderate inclination, making it so the structure is not fully visible. Overall the galaxy has an organized look, although there is a presence of disturbances. 
