The galaxy presents as a spiral type, with a prominent, moderately sized bulge. The spiral arms are well-defined, exhibiting a two-armed structure. There appears to be a medium winding to the spiral structure with a tightly wound bulge. The galaxy exhibits a slight asymmetry, suggesting possible minor disturbances from a previous or ongoing interaction, but there is no evidence of a significant merger event. The galaxy appears to have a fairly tightly packed disk with a slightly elliptical shape.
