The galaxy presents as a face-on or slightly inclined spiral. It exhibits a relatively bright, moderately sized bulge dominating its central region, with a yellow-white hue suggesting a population of older stars. Fainter spiral arms appear to emanate from the central region, displaying a clumpy morphology characteristic of active star formation regions. A strong bar structure seems present, bisecting the central bulge and extending into the inner disk, and the spiral arms originate from the ends of this bar. Overall, the galaxy displays a moderate disk and a lack of major disturbances or merging features. The galaxy is likely a late-type spiral galaxy with ongoing star formation.
