The galaxy presents a morphology consistent with a spiral type. It exhibits a bright, moderately sized central bulge. Two prominent spiral arms emanate from the central region, tracing a relatively tightly wound structure. The arms appear somewhat flocculent, exhibiting a clumpy distribution of star-forming regions. These regions are delineated by a subtle bluish tint, indicative of a younger stellar population. The overall color suggests ongoing, albeit moderate, star formation activity within the disk. There is no obvious evidence of a strong bar structure. The disk is viewed at a moderate inclination. No major signs of mergers are apparent, but some asymmetries may indicate minor disturbances. The galaxy has an overall size consistent with a dwarf spiral galaxy.
