The galaxy presents as a spiral type, characterized by a bright central bulge and a well-defined disk. Three spiral arms are visible, tightly wound around the galactic center. The bulge appears yellowish-white, with a moderate size relative to the disk, suggesting a substantial population of older stars. The arms show clumpy regions of bluish light, indicative of ongoing star formation within HII regions. The disk's ellipticity is moderate, implying a viewing angle that is somewhat inclined relative to face-on. No significant bar structure is discernible. The overall morphology suggests a relatively undisturbed spiral galaxy undergoing active star formation in its spiral arms. There are no indications of major tidal disturbances or interactions with other galaxies.
