The galaxy presents as a relatively face-on spiral with a notable central bulge. The bulge appears yellowish, suggesting an older stellar population. Fainter, less defined spiral arms extend from the central region. These arms appear somewhat clumpy and exhibit subtle color variations, hinting at regions of ongoing star formation, possibly with HII regions or young star clusters embedded within. The galaxy's disk is relatively smooth, with no obvious strong dust lanes or morphological disturbances. A general impression of the galaxy's luminosity suggests a moderately massive system with a considerable rate of star formation.
