The observed galaxy presents as a relatively well-defined spiral structure. Two prominent spiral arms are visible, exhibiting a somewhat flocculent morphology. The arms appear loosely wound, emanating from a central bulge. The bulge appears relatively small compared to the overall disk size. The dust lanes are visible within the spiral arms, particularly along the inner edges. There is evidence of active star formation within the arms, indicated by the presence of bright, localized regions of bluer light. The galaxy has an overall oblate shape. Based on the appearance of distorted light at the ends of the galaxy arms, this may be a late-stage merging galaxy with a small secondary object.
