The galaxy presents as a spiral type, observed at a slight angle relative to face-on. A dominant, bright central bulge is apparent, surrounded by a disk component. The spiral arms are well-defined and exhibit a tightly wound morphology. Evidence suggests the presence of a strong bar structure bisecting the bulge region. The disk displays a mottled texture, potentially indicative of star-forming regions. The overall color is suggestive of a moderate redshift. The galaxy appears relatively isolated.