The galaxy presents as a spiral galaxy, observed at a slight angle from face-on. The structure reveals loosely defined spiral arms extending from a central bulge. The arms exhibit a somewhat flocculent nature with moderate star formation indicated by the blue-ish color in the arms. The central bulge appears moderately sized and luminous with a yellowish hue, which suggests an older stellar population. There is no indication of a strong bar structure. The overall morphology suggests a galaxy that is not currently undergoing a major merging event, though subtle distortions in the outer disk may indicate a minor interaction in the past.
