The galaxy presents a prominent disk structure, oriented approximately face-on to our line of sight. Well-defined spiral arms emanate from the central region, displaying a two-armed morphology. The winding of the spiral arms appears to be of an intermediate type, neither tightly wound nor exceptionally loose. The stellar population within the spiral arms exhibits a clumpy distribution. These regions of higher stellar density are indicative of ongoing or recent star formation. The central bulge is of moderate size compared to the disk and exhibits a smoothly distributed, yellowish-orange luminosity profile, which is suggestive of an older stellar population. There is no prominent bar structure visible. No significant tidal features or morphological disturbances that would suggest a recent major merger event are observed, however there may be minor disturbances present.
