The galaxy presents a morphology consistent with a spiral galaxy viewed at a relatively high inclination. Faint spiral arms are visible emanating from a central bulge. The arms appear somewhat tightly wound. The overall color profile suggests active star formation, particularly within the spiral arms, giving them a patchy, flocculent appearance. The central bulge displays a smoother, more uniform color distribution, potentially indicative of an older stellar population. No obvious bar structure is apparent. There are some disturbances within the structure, though it seems unlikely there are any ongoing major merging events.