The galaxy presents as a spiral type, viewed at an angle close to face-on. Two distinct spiral arms are clearly visible, exhibiting a tightly wound morphology. A relatively prominent central bulge is present, appearing moderately sized in relation to the overall galactic disk. The color profile suggests ongoing star formation within the spiral arms. The central bulge exhibits a yellower hue, suggestive of an older stellar population. There is no clear evidence of any significant interaction or merging events affecting the galaxy’s structure, although there are some areas of disturbance. The overall color indices derived from the DECaLS photometry indicates the presence of an evolved stellar population.
