The galaxy presents as a spiral type, with discernible arm structures emanating from a central region. The arms exhibit a clumpy morphology, suggestive of active star formation regions. The overall color profile indicates a dominant blue hue, particularly concentrated within the spiral arms, which suggests a significant population of young, hot stars. There is evidence of a stellar bar structure crossing the central region. A moderate bulge is observed. There might be an ongoing minor interaction or disturbance with a neighboring galaxy, which could potentially be a tidal feature or minor merger. 
