The galaxy presents as a spiral type with a distinct, albeit not perfectly symmetrical, disk structure.  Two prominent spiral arms emanate from a central bulge. The arms appear tightly wound near the core and become less so as they extend outwards. Star formation regions are evident within the arms, indicated by localized areas of brighter, bluer light. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. There are indications of a possible bar structure present, though it is not overly prominent. Minor disturbances are visible in the arm structure, potentially indicating interactions or ongoing mergers. Overall, the galaxy seems to be actively forming stars within its spiral arms and has a moderate-sized central bulge.
