The galaxy presents as a spiral type, with noticeable arm structures extending from a central bulge region. The spiral arms are not tightly wound, displaying a more open morphology. These arms exhibit a patchy distribution of luminosity, suggesting variations in stellar populations or dust obscuration along their lengths. The central bulge appears moderately bright and concentrated, but not exceptionally dominant relative to the disk. There is some evidence of a bar-like structure bisecting the bulge, although it is not strongly defined. The overall color of the galaxy is bluish, suggesting a relatively high population of young, hot stars and ongoing star formation activity, particularly within the spiral arms. Some irregularities in the outer disk morphology may indicate minor gravitational interactions with neighboring galaxies. There is no clear evidence of a major merger event, but disturbances in the arm structure hint at past interactions. The galaxy is not viewed completely edge-on, showing a significant portion of its disk structure.
