The galaxy presents as a spiral type, viewed at an angle between face-on and edge-on. It exhibits a prominent, moderately bright central bulge, which appears slightly elongated. The disk component is well-defined and appears to be the dominant structural feature. There are multiple spiral arms visible, tightly wound around the central bulge. The arms display variations in color, with bluer regions suggestive of active star formation. The spiral arms are relatively smooth in texture with no clear major disturbances, though there are some indications of minor irregularities in their structure. There is evidence of a weak bar-like structure. The overall color index suggests a relatively active galaxy with a considerable amount of star formation occurring within the spiral arms. The galaxy appears relatively isolated with no other galactic objects in immediate proximity that would suggest a merger event.
