The galaxy presents as a spiral type, with a discernible disk structure. Spiral arms are visible, exhibiting a somewhat flocculent morphology with regions of increased stellar density and possible HII regions, especially noted in the DESI R band. The arms appear moderately wound. A central bulge is present, exhibiting a yellow hue and a gradient transition to the blue-dominated spiral arms. The bulge constitutes a significant portion of the galaxy's overall luminosity but does not heavily dominate the galaxy’s mass. There is some suggestion of a bar feature spanning much of the disk’s diameter, although not particularly prominent. The overall shape is relatively symmetric, with no evidence of major mergers or strong tidal interactions, though some minor disturbances may be indicated by the irregular distributions within the disk. The galaxy exhibits a moderate degree of inclination relative to our line of sight, allowing for a clear observation of the disk structure and spiral arm morphology. The color gradient suggests ongoing star formation, with the spiral arms showing evidence of relatively young, massive stars, and the bulge indicative of an older stellar population.
