The galaxy presents as a spiral with a well-defined disk structure, although viewed somewhat obliquely. The arms appear to be fairly tightly wound. Within the disk, clumpy regions suggestive of active star formation are visible. The central bulge of the galaxy is moderately prominent. There is evidence of a bar structure transecting the central bulge. The overall color suggests a mix of stellar populations, with both older, redder stars and younger, bluer stars present. There is no obvious sign of major interactions or recent mergers, although some minor disturbances cannot be ruled out.
