The galaxy presents a moderately inclined disk structure. The central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population. Fainter, diffuse blue light is observed in the outer regions of the disk, hinting at more recent star formation activity. The overall morphology leans towards a spiral galaxy classification, although the spiral arms are not well-defined or tightly wound. There is a suggestion of some minor disturbance to the galaxy's overall shape, but no major mergers or tidal tails are apparent.
