The object appears to be a spiral galaxy exhibiting a central bulge and a disk. The disk shows evidence of spiral arm structure, though the resolution limits a detailed characterization of the arms themselves. They appear somewhat patchy in color distribution. The central bulge is a dominant feature, appearing bright and slightly elongated, suggestive of a bar-like structure. The disk's inclination is such that it is not viewed perfectly edge-on, allowing some observation of its spiral structure. The light distribution suggests a higher concentration of older stellar populations within the bulge, while the disk contains regions of ongoing star formation. There is faint suggestion of interaction with a smaller object. Overall, this galaxy displays characteristics of a barred spiral with moderate star formation activity and signs of gravitational disturbance.
